2024-03-29T10:13:20Zhttp://cds.unistra.fr:443/reg-bin/vizier/oai.plivo://CDS.VizieR/registry2019-06-21T18:30:00Zivo_managedVizieR publishing registryVizieR_registryivo://CDS.VizieR/registryCDS VizieR serviceSebastien DerriereFrancois Ochsenbein2007-10-042015-02-021.0CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@astro.unistra.frRegistryThis registry provides access to resources from the VizieR catalogues.http://vizier.u-strasbg.frOrganisationResearchhttp://cdsweb.u-strasbg.fr/reg-bin/vizier/oai.pl100falseCDS.VizieRCDSCDS.SIMBADivo://CDS.VizieR2019-06-21T18:30:00Zivo_managedVizieR AuthorityVizieRivo://CDS.VizieRCentre de Donnees astronomiques de StrasbourgSebastien Derriere2007-10-042015-02-02CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@astro.unistra.frCataloguesThis describes CDS as the owner as CDS.VizieR authority.http://cdsweb.u-strasbg.frOrganisationResearchCentre de Donnees astronomiques de Strasbourgivo://CDS2019-06-21T18:30:00Zivo_managedCDS AuthorityCDSivo://CDSCentre de Donnees astronomiques de StrasbourgSebastien Derriere2017-10-202017-10-20CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@astro.unistra.frData centerThis authority manages CDS resources which are not part of VizieR.http://cdsweb.u-strasbg.frOrganisationResearchCentre de Donnees astronomiques de Strasbourgivo://CDS.SIMBAD/TAP2019-06-21T18:30:00Zivo_managedSIMBAD TAP query engineSIMBAD TAPivo://CDS.SIMBAD/TAPCDS SIMBAD serviceSebastien DerriereGregory Mantelet2012-05-102015-02-021.0CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@astro.unistra.frTAPThis service provides TAP access to a simplified view of the SIMBAD databasehttp://simbad.u-strasbg.frOrganisationResearchhttp://simbad.u-strasbg.fr:80/simbad/sim-tap/availabilityhttp://simbad.u-strasbg.fr:80/simbad/sim-tap/capabilitieshttp://simbad.u-strasbg.fr:80/simbad/sim-tap/tableshttp://simbad.u-strasbg.fr:80/simbad/sim-tapADQL2.0ADQL 2.0text/xmlvotableapplication/jsonjsontext/csvcsvtext/tsvtsvtext/plaintext432000432000360036002000020002000ivo://CDS.VizieR/TAP2019-06-21T18:30:00Zivo_managedTAP VizieR query engineTAPVizieRivo://CDS.VizieR/TAPCDS VizieR serviceGilles LandaisGregory Mantelet, Gilles Landais2015-02-022015-05-181.0CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@astro.unistra.frTAPThis service provides TAP access to a simplified view of the VizieR databasehttp://vizier.u-strasbg.fr/viz-bin/VizieROrganisationResearchhttp://tapvizier.u-strasbg.fr/TAPVizieR/tap/availabilityhttp://tapvizier.u-strasbg.fr/TAPVizieR/tap/capabilitieshttp://tapvizier.u-strasbg.fr/TAPVizieR/tap/tableshttp://tapvizier.u-strasbg.fr/TAPVizieR/tapADQL2.0ADQL 2.0text/xmlvotableapplication/jsonjsontext/csvcsvtext/tsvtsvtext/plaintext432000604800720086400100000000010000000001000010000ivo://CDS.VizieR/siap2019-06-21T18:30:00Zivo_managedVizieR SIA serviceVizieR SIAivo://CDS.VizieR/siapCDS VizieR serviceGilles LandaisLaurent Michel, Gilles Landais2016-04-202016-05-051.0CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@astro.unistra.frSIA, imagesThis service provides SIA access for VizieR associated data in FITS format.http://vizier.u-strasbg.fr/ArchiveResearchhttp://cdsarc.u-strasbg.fr/saadavizier/siaservice?collection=[vizier]&GETPointed360.0180.0360.0180.0ivo://CDS.VizieR/ssap2019-06-21T18:30:00Zivo_managedVizieR SSA serviceVizieR SSAivo://CDS.VizieR/ssapCDS VizieR serviceGilles LandaisLaurent Michel, Gilles Landais2016-04-202016-05-271.0CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@astro.unistra.frSSA, spectra, sed, time-seriesThis service provides SSA access for VizieR associated data in FITS/VOTable format.http://vizier.u-strasbg.fr/ArchiveResearchhttp://cdsarc.u-strasbg.fr/saadavizier/ssaservice?collection=[vizier]&GETapplication/x-votable+xmlquerycustomarchivalICRS180999999100180http://cdsarc.u-strasbg.fr/assocdata/ivo://CDS.VizieR/ObsTAP2019-06-21T18:30:00Zivo_managedTAP VizieR query engineTAPVizieRivo://CDS.VizieR/ObsTAPCDS VizieR serviceGilles LandaisLaurent Michel, Gilles Landais2018-10-212019-06-121.0CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@astro.unistra.frObsTAPThis service provides ObsTAP access to VizieR spectra, time-series and images.http://vizier.u-strasbg.fr/viz-bin/VizieRArchiveResearchhttp://cdsarc.u-strasbg.fr/saadavizier.tap/tap/availabilityhttp://cdsarc.u-strasbg.fr/saadavizier.tap/tap/capabilitieshttp://cdsarc.u-strasbg.fr/saadavizier.tap/tap/tableshttp://cdsarc.u-strasbg.fr/saadavizier.tap/tapADQL2.0ADQL 2.0text/xmlvotableapplication/jsonjsontext/csvcsvtext/plaintext8640086400360036001000001000000ivo://CDS/aladin/hipsmaster2019-06-21T18:30:00Zivo_managedCDS image/cube HiPS service (master server)CDS hipsmasterivo://CDS/aladin/hipsmasterCDSCentre de Donnees astronomiques de strasbourgPierre Fernique2017-10-182017-10-201.0CDS Helpdesk
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@astro.unistra.frCDS image/cube HiPS serviceThe CDS provides a collection of reference surveys available thanks to HiPS protocol.http://aladin.u-strasbg.fr/hipsArchiveResearchhttp://alasky.u-strasbg.fr/hipslistGETivo://CDS/aladin/hipsslave2019-06-21T18:30:00Zivo_managedCDS image/cube HiPS service (slave server)CDS hipsslaveivo://CDS/aladin/hipsslaveCDSCentre de Donnees astronomiques de strasbourgPierre Fernique2017-10-182017-10-201.0CDS Helpdesk
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@astro.unistra.frCDS image/cube HiPS serviceThe CDS provides a collection of reference surveys available thanks to HiPS protocol.http://aladin.u-strasbg.fr/hipsArchiveResearchhttp://alaskybis.u-strasbg.fr/hipslistGEThttps://alaskybis.u-strasbg.fr/hipslistGETivo://CDS/vizier/hipsserver2019-06-21T18:30:00Zivo_managedCDS catalog HiPS ServiceCDS catalog HiPSivo://CDS/vizier/hipsserverCDSCentre de Donnees astronomiques de strasbourgPierre Fernique2017-10-182017-10-201.0CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@astro.unistra.frCDS image/cube HiPS serviceThe CDS provides a collection of reference catalogs available thanks to HiPS protocol.http://aladin.u-strasbg.fr/hipsArchiveResearchhttp://axel.u-strasbg.fr/HiPSCatService/hiplistGETivo://CDS.VizieR/I/1342019-06-21T18:30:00ZIivo_managed1Trapezium Multiple Systems (Salukvadze, 1978)I/134ivo://CDS.VizieR/I/134CDSSalukvadze G.N.Francois Ochsenbein [CDS]1997-12-09T10:59:5111-Feb-1997CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frMultiple_StarsThe present catalogue of Trapezium-type Multiple Systems was compiled on the basis of the Index Catalogue of Visual Binary Stars (IDS, Jeffers et al., 1963). At the period of compilation of the Abastumani catalogue, IDS was the most complete catalogue concerning not only stars, but also the data on double stars. Besides giving relative positions, IDS presents the coordinates at 1900 and 2000 epochs, as well as in most cases magnitudes, spectral classes and proper motions. IDS contains all double and multiple stars from the North to the South poles with relative positions published up to the end of 1960, their total number being 64247. In order to select optimum value of K (ratio of the largest to the smallest distances among the components), which is the main criterion for relating a multiple star to the trapezium type, the dependence of the observed trapezia number on the K value has been analysed, and the value 2.6 adopted for it. To exclude optical components, upper limits for the distances of faint components to the main star have been introduced, and the components fainter than 12.5mag were excluded altogether (Salukvadze, 1978). The catalogue of Trapezium-type Multiple Systems contains 412 trapezia, for which, after examining all main spectral catalogues (Jaschek et al., 1964; Kennedy et al., 1974; Houck et al., 1975; Cruz-Gonzales et al., 1974; Lindsey et al., 1968), spectral classes in the MK system have been specified. This was done for 100 systems, including 65 stars of O and B spectral classes. The following data on trapezia are given in the catalogue: positional angles and distances, magnitudes and spectral classes according to HD as well as MK, the ADS and BD identification number of the main star. On the basis of the probability, deduced by Ambartsumian (1954), the number of pseudo-trapezia was estimated, that is, the number of multiple stars, which in fact have no trapezium-type configurations, but are observed as trapezia as a result of their projection on the celestial sphere. The number of estimated pseudo-trapezia is 167. It should be mentioned that among 59 trapezia, the main components of which are of the O-B2 spectral class, there are only 5 pseudo-trapezia. This enables us to maintain that there is a considerable percent of real trapezia among the ones of mentioned spectral classes. Evaluation of the number of optical systems, formed as a result of the appearance of background stars in circles, which are determined by the upper limits of components' distances, led to their insignificant number 9. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?I/134CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=I/134http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=I/134GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
I/134/dataThe Catalogue of Trapezium Multiple SystemsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordMainFlag[*] The asterisk indicates the main star of a trapezium systemmeta.noteSeqOrdinal numbermeta.id;meta.mainIDSDesignation in "Index Catalogue of Visual Double Stars" (based on B1900 position)meta.idCompDesignation of componentsmeta.idtheta[0/360] Positional angle of a component relative to the main stardegpos.posAngrhoDistance of a component to the main stararcsecpos.angDistance;src.orbitalVmag1? Magnitude of the main star (1)magphot.magVmag2? Magnitudes of trapezium componentmagphot.mag;em.opt.VSp1IDS Spectral class of the main star (1)src.spTypeSpType1Spectral class of the main star in the MK system (1)src.spTypeADS? ADS number (1)meta.idDMDurchmusterung number (1)meta.id
ivo://CDS.VizieR/I/1502019-06-21T18:30:00ZIivo_managed1Proper Motions for High Luminosity Stars (Valitova+ 1990)I/150ivo://CDS.VizieR/I/150CDSValitova A.M., Karimova D.K., and Pavlovskaya E.D.Julie Anne Watko [SSDOO/ADC]1997-12-09T11:05:4120-May-1996CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frStarsProper_MotionsMeridian circle observations of high luminosity stars were used to supplement previous positions to derive improved proper motions. The proper motions and positions are derived for J2000.0 and for the epoch of observation but the systematic correction: FK5-FK4 and the correction to FK5 for each star were ignored. V magnitudes and MK spectral types are taken from published catalogs. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?I/150CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=I/150http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=I/150GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table I/150/catalog (The catalogue)http://vizier.u-strasbg.fr/viz-bin/conesearch/I/150/catalog?GETtext/xml+votable18050000true63.2153320312499922.4272727657409130.028629053431811713http://alasky.u-strasbg.fr/footprints/cats/vizier/I/150?product=MOC&nside=512Optical
I/150/catalogThe cataloguerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordSeq[1/309]+ Sequential numbermeta.id;meta.mainHD*Number in HD cataloguemeta.idSpMK spectral and luminosity classsrc.spTypeVmagV magnitudemagphot.mag;em.opt.VRAJ2000*Right Ascension (J2000.0) hours"h:m:s"pos.eq.ra;meta.mainDEJ2000*Declination (J2000.0) sign"d:m:s"pos.eq.dec;meta.mainpmRAProper motion in RA equinox J2000.0 (J years)s/apos.pm;pos.eq.rae_pmRAError of pmRA (J years)s/astat.errorEpRAEpoch of observations for RA (B years)atime.epochcatRA*Number of catalogues RAmeta.numberpmDEProper motion in DE equinox J2000.0 (J years)arcsec/apos.pm;pos.eq.dece_pmDEError of pmDEarcsec/astat.errorEpDEEpoch of observations for DE (B years)atime.epochcatDE*Number of catalogues DEmeta.number
ivo://CDS.VizieR/I/2062019-06-21T18:30:00ZIivo_managed1Bright Stars Supplement to PPM (Bastian+ 1993)I/206ivo://CDS.VizieR/I/206CDSBastian U., Roeser S.Joseph Florsch [CDS] and Gail Schneider [NSSDC/ADC]1997-12-09T13:39:3509-Nov-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPositional_DataProper_MotionsA number of bright stars is missing from the PPM Star Catalogue, both on the northern <I/146> and on the southern <I/193> hemisphere. The Bright Stars Supplement described here makes PPM complete down to V=7.5 mag. For this purpose it lists all missing stars brighter than V=7.6 mag that we could find in published star lists. Their total number is 275. Only 2 of them are brighter than V=3.5. This replaces the December 1992 edition (catalogue I/194) of the Bright Stars Supplement which inadvertently contained 46 duplicates of stars already contained in the main parts of PPM. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?I/206CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=I/206http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=I/206GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table I/206/ppmb (The Bright Star Supplement)http://vizier.u-strasbg.fr/viz-bin/conesearch/I/206/ppmb?GETtext/xml+votable18050000true62.2265625000000123.094735814402510.028629053431811713Opticalhttp://alasky.u-strasbg.fr/footprints/cats/vizier/I/206?product=MOC&nside=512
I/206/ppmbThe Bright Star SupplementrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordPPM[400001/400321]+ PPM numbermeta.id;meta.mainDMDurchmusterung, here emptymeta.idMagVisual magnitudemagphot.mag;em.opt.VSpSpectral type (blank)src.spTypeRAJ2000Right Ascension for the Equinox=J2000.0 and Epoch=J2000.0, on the system of FK5"h:m:s"pos.eq.ra;meta.mainDEJ2000Declination J2000 (sign)"d:m:s"pos.eq.dec;meta.mainpmRAProper motion in right ascensions/apos.pm;pos.eq.rapmDEProper motion in declinationarcsec/apos.pm;pos.eq.decNpos[0] Number of individual positions usedmeta.numbere_RA[99] Mean error of RA multiplied by cos(DE)10masstat.errore_DE[99] Mean error of DE10masstat.errore_pmRA[9.9] Mean error of pmRA multiplied by cos(DE)mas/astat.errore_pmDE[9.9] Mean error of proper motion in DEmas/astat.errorEpRA-1900[50] Weighted mean epoch for RA, given in years since 1900atime.epochEpDE-1900[50] Weighted mean epoch for DE, given in years since 1900atime.epochFlag1[B] 'B' for Bright starmeta.noteFlag2[D] 'D' for double starmeta.noteFlag5[R] 'R' for Remark (only No 400148) explained in file descripmeta.note
ivo://CDS.VizieR/I/2122019-06-21T18:30:00ZIivo_managed1Proper motions in NGC 3680 (Kozhurina-Platais+, 1995)I/212ivo://CDS.VizieR/I/212CDSKozhurina-Platais V., Girard T.M., Platais I., van Altena W.F., Ianna P.A., Cannon R.D.Francois Ochsenbein [CDS]1997-12-09T14:54:3608-Feb-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPositional_DataOpen_ClustersProper_MotionsA catalogue of positions, proper motions and photographic BV magnitudes for 2711 stars in and around the open cluster NGC 3680 is presented. The Catalogue is complete down to B=17.5 mag in a rectangular, one square degree area centered on the cluster. The limiting magnitude of the Catalogue is B=18.4 mag. The mean standard error of the proper motions for well-measured stars is +/-0.35 mas/yr. The photographic B and V magnitudes are accurate to about +/-0.1 mag. The mean error of the relative positions for all 2711 is +/-0.025 arcsec at the mean epoch of the plate material, 1977.8. For each star, three different cluster membership estimators are presented. For convenience, cross-identifications to other studies are provided. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?I/212CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=I/212http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=I/212GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table I/212/ngc3680 (The catalogue of stars in NGC 3680)http://vizier.u-strasbg.fr/viz-bin/conesearch/I/212/ngc3680?GETtext/xml+votable18050000true171.6793313069909-43.6554461641832460.028629053431811713Opticalhttp://alasky.u-strasbg.fr/footprints/cats/vizier/I/212?product=MOC&nside=512
I/212/xidCross-identifications with previous workrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNo[1/2711]+= The present Catalogue number.meta.id;meta.mainAnt-TwaIdentification with Anthony-Twarog et al. (1991).meta.id.crossEggenIdentification with Eggen (1969).meta.id
I/212/ngc3680The catalogue of stars in NGC 3680recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNo[1/2711]+ Sequential number of the star.meta.id;meta.mainVmag[7/18] Photographic BV-photometry.magphot.mag;em.opt.VB-VPhotographic colour indexmagphot.color;em.opt.B;em.opt.VRAJ2000[11] Right Ascension (hours) Equinox=J2000, Epoch=J2000"h:m:s"pos.eq.ra;meta.mainDEJ2000[-] Declination J2000 (sign)"d:m:s"pos.eq.dec;meta.mainnPlatesThe number of plates used in the proper motion calculation.meta.numberpmXRelative proper motions in X-coordinate.mas/yrpos.pmpmYRelative proper motions in Y-coordinate.mas/yrpos.pme_pmXFormal error of pmX.mas/yrstat.errore_pmYFormal error of pmY.mas/yrstat.errorPr(pm)[0/100] Standard membership probability for the cluster NGC 3680. (2)%stat.fit.goodnessPr(pm,r)[0/100] Joint spatial/proper motion membership probability. (2)%stat.fit.goodnessPr(S)[0/100]? Local-sample membership probability; negative probabilities indicate a not computed probability. (2)%stat.fit.goodnessXStandard-plate coordinate (1)mmpos.cartesian.x;instr.detYStandard-plate coordinate (1)mmpos.cartesian.y;instr.dete_XMean error on X (microns)umstat.errore_YMean error on Y (microns)umstat.error
ivo://CDS.VizieR/I/2212019-06-21T18:30:00ZIivo_managed1The Magellanic Catalogue of Stars - MACS (Tucholke+ 1996)I/221ivo://CDS.VizieR/I/221CDSTucholke H.-J., de Boer K.S., Seitter W.C.Hans-Joachim Tucholke [Univ. Bonn]1997-12-09T15:08:3420-Nov-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPositional_DataThe Magellanic Catalogue of Stars (MACS) is based on scans of ESO Schmidt plates and contains about 244,000 stars covering large areas around the LMC and the SMC. The limiting magnitude is B<16.5m and the positional accuracy is better than 0.5" for 99% of the stars. The stars of this catalogue were screened interactively to ascertain that they are undisturbed by close neighbours. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?I/221CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=I/221http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=I/221GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table I/221/lmc (The Large Magellanic Cloud)http://vizier.u-strasbg.fr/viz-bin/conesearch/I/221/lmc?GETtext/xml+votable18050000true83.85245901639344-77.434200597692180.028629053431811713Cone search capability for table I/221/smc (The Small Magellanic Cloud)http://vizier.u-strasbg.fr/viz-bin/conesearch/I/221/smc?GETtext/xml+votable18050000true28.8031914893617-77.08943233063140.028629053431811713http://alasky.u-strasbg.fr/footprints/cats/vizier/I/221?product=MOC&nside=512Optical
I/221/smcThe Small Magellanic CloudrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordMACSDesignationmeta.id;meta.mainRAJ2000Right Ascension J2000 , Epoch 1989.0 (hours)"h:m:s"pos.eq.ra;meta.mainDEJ2000Declination J2000 (sign)"d:m:s"pos.eq.dec;meta.mainNposNumber of positions usedmeta.numberMag[]? Instrumental Magnitude (to be used only in a relative sense)magphot.magPosFlag[0/1] Position Flag (0: ok, 1: internal error larger than 0.5")meta.codeMagFlag[0/1] Megnitude Flag (0: ok, 1: bad photometry or possible variable)meta.code;src.varBochumFlag*[0] Bochum Flagmeta.code
I/221/lmcThe Large Magellanic CloudrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordMACSDesignationmeta.id;meta.mainRAJ2000Right Ascension J2000 , Epoch 1989.0 (hours)"h:m:s"pos.eq.ra;meta.mainDEJ2000Declination J2000 (sign)"d:m:s"pos.eq.dec;meta.mainNposNumber of positions usedmeta.numberMag[]? Instrumental Magnitude (to be used only in a relative sense)magphot.magPosFlag[0/1] Position Flag (0: ok, 1: internal error larger than 0.5")meta.codeMagFlag[0/1] Megnitude Flag (0: ok, 1: bad photometry or possible variable)meta.code;src.varBochumFlag*[0] Bochum Flagmeta.code
ivo://CDS.VizieR/I/2332019-06-21T18:30:00ZIivo_managed1Orbital Elements of Minor Planets 1997 (Batrakov+ 1996)I/233ivo://CDS.VizieR/I/233CDSBatrakov Yu.V., Shor V.A.Francois Ochsenbein [CDS]1997-12-09T15:34:5011-Jul-1996CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPlanets+AsteroidsThe catalogue contains osculating elements of all permanently numbered minor planets as of November 7, 1995. The elements are given with respect to the ecliptic plane and equinox J2000 for the standard epoch JD2450800.5 = 1997 December 18.0 ET. The elements of (719) Albert which is considered to be lost are given for the epoch when the planet was discovered. The catalogue data, in general, correspond to those published in "Ephemerides of Minor Planets for 1997", St.Petersburg, 1996. Along with these data the catalogue incorporates some connected information. (C) Copyright 1996 ITA RAS http://cdsarc.u-strasbg.fr/cgi-bin/Cat?I/233CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=I/233http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=I/233GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tap
I/233/catalogThe ElementsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordPlanet[1/6678]+ Minor Planet numbermeta.idEquinox[2000] equinox = 2000 (2000.0)atime.equinoxEpepoch (year) (1)"Y:M:D"time.epochMmean anomalydegsrc.orbital.meanAnomalyomegaargument of periheliondegsrc.orbital.periastronNodenodedegsrc.orbital.nodeiinclination to the eclipticdegsrc.orbital.inclinationeeccentricitysrc.orbital.eccentricitydmotionmean daily motiondeg/dphys.veloc.angHabsolute magnitude, H (2)magphys.magAbs;em.optG? slope parameter, G (2)stat.fit.paramNoppnumber of oppositions used for improvementmeta.numberNobsnumber of observations used for improvementmeta.numberYear1the first year of the time interval covered by the observations used for improvementatime.epochYear2the last year of the time interval covered by the observations used for improvementatime.epochrms? Mean-root-square or maximum residual (4)arcsecstat.errorSourcecode for the source of elements (5)meta.refNamename or preliminary designation of the planetmeta.id;meta.mainAuthorauthor of the elementsmeta.bib.authorUnum[0/9]? Uncertainty number (6)meta.codeDatesix-figure code of the date when the elements have been recorded in the ITA"Y:M:D"time.epoch
ivo://CDS.VizieR/I/2412019-06-21T18:30:00ZIivo_managed1The N70E catalogue (Kolesnik, 1997)I/241ivo://CDS.VizieR/I/241CDSKolesnik Y.B.Yuri Kolesnik [Inst. Astronomy Moscow]1997-12-09T15:37:041997-Mar-28CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPositional_DataProper_MotionsThe N70E catalogue provides improved mean positions and proper motions for the 718 Basic fundamental stars from the FK5 catalogue in the equatorial zone covering the declination range from -30 to +30 degrees. The catalogue is resulted from revision of the FK5 system on the basis of 36 modern absolute and quasi-absolute catalogues and the four fundamental catalogues FK3, FK4, GC, N30, and revision of FK5 individual positions and proper motions by use of 52 catalogues distributed at the time span from 1900 to 1993. Absolute orientation in space of N70E catalogue is defined by the IAU (1976) system of astronomical constants. Only the machine-readable version of the N70E catalogue is distributed. It contains the positions and proper motions of the stars for the epoch and equinox J2000.0, the mean epochs of individual observed right ascensions and declinations used to determine the final positions, and the mean errors of the final positions and proper motions for the reported epochs. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?I/241CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=I/241http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=I/241GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table I/241/n70e (*The N70E catalogue)http://vizier.u-strasbg.fr/viz-bin/conesearch/I/241/n70e?GETtext/xml+votable18050000true45.57128906254.0880300560850960.028629053431811713http://alasky.u-strasbg.fr/footprints/cats/vizier/I/241?product=MOC&nside=512Optical
I/241/n70e*The N70E cataloguerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordFK5*FK5 numbermeta.id;meta.mainRAJ2000Right ascension hours (J2000.0)"h:m:s"pos.eq.ra;meta.mainpmRACentennial proper motion in RA (J2000.0)0.01s/yrpos.pm;pos.eq.raDEJ2000Sign of declination (Dec) (J2000.0)"d:m:s"pos.eq.dec;meta.mainpmDEProper motion in DE (J2000.0)0.01arcsec/yrpos.pm;pos.eq.decEpRA-1900*Mean Epoch of individual observed RAyrtime.epoche_RAs*Mean error in individual observed RA0.01arcsecstat.errore_pmRA*Mean error in individual observed pmRA0.1mas/yrstat.errorEpDE-1900*Mean Epoch of individual observed DEyrtime.epoche_DEs*Mean error in individual observed DE0.01arcsecstat.errore_pmDE*Mean error in individual observed pmDE0.1mas/yrstat.error
ivo://CDS.VizieR/I/2452019-06-21T18:30:00ZIivo_managed1Orbital Elements of Minor Planets 1998 (Batrakov+ 1997)I/245ivo://CDS.VizieR/I/245CDSBatrakov Yu.V., Shor V.A.V.A.Shor [ITA], Francois Ochsenbein [CDS]1997-12-09T15:38:0118-Jul-1997CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPlanets+AsteroidsThe catalogue contains osculating elements of all permanently numbered minor planets as of November 25, 1996. The elements are given with respect to the ecliptic plane and equinox J2000 for the standard epoch JD2451000.5 = 1998 July 6.0 ET. The elements of (719) Albert which is considered to be lost are given for the epoch when the planet was discovered. The catalogue data, in general, correspond to those in "Ephemerides of Minor Planets for 1998", St.Petersburg, 1997 (in print). Along with these data the catalogue incorporates some connected information. (C) Copyright 1997 ITA RAS http://cdsarc.u-strasbg.fr/cgi-bin/Cat?I/245CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=I/245http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=I/245GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tap
I/245/catalogThe ElementsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordPlanet[1/7316]+ Minor Planet numbermeta.idEquinox[2000] equinox = 2000 (2000.0)atime.equinoxEpepoch (year) (1)"Y:M:D"time.epochMmean anomalydegsrc.orbital.meanAnomalyomegaargument of periheliondegsrc.orbital.periastronNodenodedegsrc.orbital.nodeiinclination to the eclipticdegsrc.orbital.inclinationeeccentricitysrc.orbital.eccentricitydmotionmean daily motiondeg/dphys.veloc.angHabsolute magnitude, H (2)magphys.magAbs;em.optG? slope parameter, G (2)stat.fit.paramNoppnumber of oppositions used for improvementmeta.numberNobsnumber of observations used for improvementmeta.numberYear1the first year of the time interval covered by the observations used for improvementatime.epochYear2the last year of the time interval covered by the observations used for improvementatime.epochrms? Mean-root-square or maximum residual (4)arcsecstat.errorSourcecode for the source of elements (5)meta.refNamename or preliminary designation of the planetmeta.id;meta.mainAuthorauthor of the elementsmeta.bib.authorUnum[0/9]? Uncertainty number (6)meta.codeDatesix-figure code of the date when the elements have been recorded in the ITA"Y:M:D"time.epoch
ivo://CDS.VizieR/II/1082019-06-21T18:30:00ZIIivo_managed1Two-Micron Sky Survey, Nearest SAO Stars on POSS (Nagy 1983)II/108ivo://CDS.VizieR/II/108CDSPrints Nagy T.A., Hill R.S., and Mead J.M.Julie Anne Watko [SSDOO/ADC]1997-12-09T15:41:4103-Nov-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frThis catalog is a list of potential guide stars developed for a program to obtain more precise positions of objects in the IRC Two-Micron Sky Survey of Neguebauer and Leighton (1969). For each IRC source (col. 1), it gives: (col. 2) the identification of the star in the SAO catalog which is nearest, (col. 3) the great circle arc distance (in seconds) between the SAO star and the IRC source, (col. 4) the position angle (in degrees) of the IRC source relative to the SAO star, (col. 5) the plate number(s) of the POSS on which the IRC source appears, (col. 6,7) the approximate rectangular coordinates (in mm) of the IRC source on the POSS print area with respect to the Southwest corner, and (col. 8) the modified Luyten Palomar number. The POSS plate numbers given are for the red plates. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?II/108CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=II/108http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=II/108GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapInfrared
II/108/dataCatalog DatarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordID? IRC Number from Two-Micron Sky Surveymeta.idSAO*? ID of Closest SAO Star to IRC Sourcemeta.idD*? Great Circle Arc Distance between SAO and IRCarcsecpos.angDistancePA*? Position Angle of IRC Relative to SAO Sourcedegpos.posAngPOSS*POSS Plate IDobs.fieldX*Rectangular Coordinate on POSS Print Areammpos.cartesian.x;instr.detYRectangular Coordinate on POSS Print Areammpos.cartesian.y;instr.detMLP*Modified Luyten Palomar Numbermeta.id
ivo://CDS.VizieR/II/1162019-06-21T18:30:00ZIIivo_managed1Photoelectric Photometry in Johnson UBVRI System (Lanz 1986)II/116ivo://CDS.VizieR/II/116CDSLanz T.Francois Ochsenbein [CDS]1997-12-09T15:42:1920-Oct-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometry:wide-bandThe catalog is a compilation of photoelectric photometry in the Johnson UBVRI system published prior to mid-1984. The catalog contains a total of 6849 stars in the original Johnson system (Morel and Magnenat 1978), 467 stars in the system of Kunkel and Rydgren (1979), 1150 stars in the system of Moffett and Barnes III (1979), and 252 stars in the system of Neckel and Chini (1980). The catalog is in 14 files: The first 12 files list observational data, mean values, and references for each of the four standard systems. An additional two files contain the numbering scheme of Mermilliod (1978) used to identify objects, and introductory information. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?II/116CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=II/116http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=II/116GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOpticalInfrared
II/116/obs-mbObservations in Moffett+Barnes systemrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordLIDObject identification in Lausanne/Geneva system (see file "codes")meta.id;meta.mainm_LID[D1-6] 'D' for unresolved binary, or component numbermeta.code.multipVarFlag[V] 'V' if star is variablemeta.noteVmag[]? V magnitude in the Johnson UBVRI systemmagphot.mag;em.opt.VU-B[]? U-B color in the Johnson UBVRI systemmagphot.color;em.opt.U;em.opt.BB-V[]? B-V color in the Johnson UBVRI systemmagphot.color;em.opt.B;em.opt.VV-R[]? V-R color in the Johnson UBVRI systemmagphot.color;em.opt.V;em.opt.RR-I[]? R-I color in the Johnson UBVRI systemmagphot.color;em.opt.R;em.opt.IImag[]? I magnitude in the Johnson UBVRI systemmagphot.mag;em.opt.In_NumObs[/*S] Qualifying code for NumObs (1)meta.noteNumObs[]? Number of observationsmeta.numberRef[8001/73007] Reference Number (file "refs")meta.ref
II/116/obs-jObservations in Johnson UBVRI systemrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordLIDObject identification in Lausanne/Geneva system (see file "codes")meta.id;meta.mainm_LID[D1-6] 'D' for unresolved binary, or component numbermeta.code.multipVarFlag[V] 'V' if star is variablemeta.noteVmag[]? V magnitude in the Johnson UBVRI systemmagphot.mag;em.opt.VU-B[]? U-B color in the Johnson UBVRI systemmagphot.color;em.opt.U;em.opt.BB-V[]? B-V color in the Johnson UBVRI systemmagphot.color;em.opt.B;em.opt.VV-R[]? V-R color in the Johnson UBVRI systemmagphot.color;em.opt.V;em.opt.RR-I[]? R-I color in the Johnson UBVRI systemmagphot.color;em.opt.R;em.opt.IImag[]? I magnitude in the Johnson UBVRI systemmagphot.mag;em.opt.In_NumObs[/*S] Qualifying code for NumObs (1)meta.noteNumObs[]? Number of observationsmeta.numberRef[8001/73007] Reference Number (file "refs")meta.ref
II/116/refsExplanations of ReferencesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordRef[8001/73007]?+ Reference Number, blank for continuation lines (1)meta.refTextText of bibliographical referencemeta.bib.bibcode
II/116/obs-ncObservations in Neckel+Chini systemrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordLIDObject identification in Lausanne/Geneva system (see file "codes")meta.id;meta.mainm_LID[D1-6] 'D' for unresolved binary, or component numbermeta.code.multipVarFlag[V] 'V' if star is variablemeta.noteVmag[]? V magnitude in the Johnson UBVRI systemmagphot.mag;em.opt.VU-B[]? U-B color in the Johnson UBVRI systemmagphot.color;em.opt.U;em.opt.BB-V[]? B-V color in the Johnson UBVRI systemmagphot.color;em.opt.B;em.opt.VV-R[]? V-R color in the Johnson UBVRI systemmagphot.color;em.opt.V;em.opt.RR-I[]? R-I color in the Johnson UBVRI systemmagphot.color;em.opt.R;em.opt.IImag[]? I magnitude in the Johnson UBVRI systemmagphot.mag;em.opt.In_NumObs[/*S] Qualifying code for NumObs (1)meta.noteNumObs[]? Number of observationsmeta.numberRef[8001/73007] Reference Number (file "refs")meta.ref
II/116/hom-ncHomogenized photometry in Neckel+Chini systemrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordLIDObject identification in Lausanne/Geneva system (see file "codes")meta.id;meta.mainm_LID[D1-6] 'D' for unresolved binary, or component numbermeta.code.multipVarFlag[V] 'V' if star is variablemeta.noteVmag[]? V magnitude in the Johnson UBVRI systemmagphot.mag;em.opt.VU-B[]? U-B color in the Johnson UBVRI systemmagphot.color;em.opt.U;em.opt.BB-V[]? B-V color in the Johnson UBVRI systemmagphot.color;em.opt.B;em.opt.VV-R[]? V-R color in the Johnson UBVRI systemmagphot.color;em.opt.V;em.opt.RR-I[]? R-I color in the Johnson UBVRI systemmagphot.color;em.opt.R;em.opt.IImag[]? I magnitude in the Johnson UBVRI systemmagphot.mag;em.opt.IWeightWeight of the photoelectric data, derived from number of measurementsstat.weight
II/116/hom-jHomogenized photometry in Johnson UBVRI systemrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordLIDObject identification in Lausanne/Geneva system (see file "codes")meta.id;meta.mainm_LID[D1-6] 'D' for unresolved binary, or component numbermeta.code.multipVarFlag[V] 'V' if star is variablemeta.noteVmag[]? V magnitude in the Johnson UBVRI systemmagphot.mag;em.opt.VU-B[]? U-B color in the Johnson UBVRI systemmagphot.color;em.opt.U;em.opt.BB-V[]? B-V color in the Johnson UBVRI systemmagphot.color;em.opt.B;em.opt.VV-R[]? V-R color in the Johnson UBVRI systemmagphot.color;em.opt.V;em.opt.RR-I[]? R-I color in the Johnson UBVRI systemmagphot.color;em.opt.R;em.opt.IImag[]? I magnitude in the Johnson UBVRI systemmagphot.mag;em.opt.IWeightWeight of the photoelectric data, derived from number of measurementsstat.weight
II/116/hom-mbHomogenized photometry in Moffett+Barnes systemrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordLIDObject identification in Lausanne/Geneva system (see file "codes")meta.id;meta.mainm_LID[D1-6] 'D' for unresolved binary, or component numbermeta.code.multipVarFlag[V] 'V' if star is variablemeta.noteVmag[]? V magnitude in the Johnson UBVRI systemmagphot.mag;em.opt.VU-B[]? U-B color in the Johnson UBVRI systemmagphot.color;em.opt.U;em.opt.BB-V[]? B-V color in the Johnson UBVRI systemmagphot.color;em.opt.B;em.opt.VV-R[]? V-R color in the Johnson UBVRI systemmagphot.color;em.opt.V;em.opt.RR-I[]? R-I color in the Johnson UBVRI systemmagphot.color;em.opt.R;em.opt.IImag[]? I magnitude in the Johnson UBVRI systemmagphot.mag;em.opt.IWeightWeight of the photoelectric data, derived from number of measurementsstat.weight
II/116/hom-krHomogenized photometry in Kunkel+Rydgren systemrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordLIDObject identification in Lausanne/Geneva system (see file "codes")meta.id;meta.mainm_LID[D1-6] 'D' for unresolved binary, or component numbermeta.code.multipVarFlag[V] 'V' if star is variablemeta.noteVmag[]? V magnitude in the Johnson UBVRI systemmagphot.mag;em.opt.VU-B[]? U-B color in the Johnson UBVRI systemmagphot.color;em.opt.U;em.opt.BB-V[]? B-V color in the Johnson UBVRI systemmagphot.color;em.opt.B;em.opt.VV-R[]? V-R color in the Johnson UBVRI systemmagphot.color;em.opt.V;em.opt.RR-I[]? R-I color in the Johnson UBVRI systemmagphot.color;em.opt.R;em.opt.IImag[]? I magnitude in the Johnson UBVRI systemmagphot.mag;em.opt.IWeightWeight of the photoelectric data, derived from number of measurementsstat.weight
II/116/obs-krObservations in Kunkel+Rydgren systemrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordLIDObject identification in Lausanne/Geneva system (see file "codes")meta.id;meta.mainm_LID[D1-6] 'D' for unresolved binary, or component numbermeta.code.multipVarFlag[V] 'V' if star is variablemeta.noteVmag[]? V magnitude in the Johnson UBVRI systemmagphot.mag;em.opt.VU-B[]? U-B color in the Johnson UBVRI systemmagphot.color;em.opt.U;em.opt.BB-V[]? B-V color in the Johnson UBVRI systemmagphot.color;em.opt.B;em.opt.VV-R[]? V-R color in the Johnson UBVRI systemmagphot.color;em.opt.V;em.opt.RR-I[]? R-I color in the Johnson UBVRI systemmagphot.color;em.opt.R;em.opt.IImag[]? I magnitude in the Johnson UBVRI systemmagphot.mag;em.opt.In_NumObs[/*S] Qualifying code for NumObs (1)meta.noteNumObs[]? Number of observationsmeta.numberRef[8001/73007] Reference Number (file "refs")meta.ref
ivo://CDS.VizieR/II/1172019-06-21T18:30:00ZIIivo_managed1Catalog of UBVRI Photometry of Globular Clusters (Peterson 1986)II/117ivo://CDS.VizieR/II/117CDSPeterson C. J.Julie Anne Watko [SSDOO/ADC]1997-12-09T15:42:2921-Feb-1996CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frGlobular_ClustersPhotometry:wide-bandPhotometric data directly obtained in UBVRI or converted to UBVRI magnitudes are tabulated. The data comprise approximately 4600 records from 56 individuals and contains data unpublished at the time of the compilation as well as published data. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?II/117CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=II/117http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=II/117GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOpticalInfrared
II/117/refsReferences (table 8)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordRefReference Codemeta.bib.bibcodeTextText of referencemeta.refNNumber of Clustersmeta.id;meta.mainTypeType of Datameta.note
II/117/dataData (tables 1-7)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordnameCluster Namemeta.id;meta.mainRef*Reference Codemeta.bib.bibcodeap? Aperture Diameterarcmininstr.fovUmag*? U Magnitudemagphot.mag;em.opt.UU-B? Johnson Ultraviolet Color Indexmagphot.color;em.opt.U;em.opt.BBmag? B Magnitude, computed from V+(B-V)magphot.mag;em.opt.BB-V? Johnson Blue Color Indexmagphot.color;em.opt.B;em.opt.VVmag? V Magnitudemagphot.mag;em.opt.VV-R? Visual-Red Color Indexmagphot.color;em.opt.V;em.opt.RRmag? R Magnitude, computed from V-(V-R)magphot.mag;em.opt.RV-I*? Visual-I Band Color Indexmagphot.color;em.opt.V;em.opt.IImag? I Magnitude, computed from V-(V-I)magphot.mag;em.opt.I
ivo://CDS.VizieR/II/124A2019-06-21T18:30:00ZIIivo_managed1UBV and MK types in Open Clusters, 3rd ed. (Mermilliod 1986)II/124Aivo://CDS.VizieR/II/124ACDSMERMILLIOD J.C.: 1986Francois Ochsenbein [CDS]1997-12-09T15:46:1211-Apr-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frOpen_ClustersSpectral_ClassificationPhotometry:wide-bandSee the complete documentation written by Anne C. Raugh (file adc.doc) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?II/124ACatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=II/124Ahttp://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=II/124AGETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
II/124A/catalogThe CataloguerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordLIDIdentification in Geneva/Lausanne system (1)meta.id;meta.mainn_LIDRemark about star (2)meta.noteOrigIDOriginal identification as listed in reference for the datameta.refpmIDIdentification as listed in proper motion studymeta.idHD[1/350100]? Henry Draper Catalog (HD) numbermeta.idDMDurchmusterung catalog ID (3)meta.idVmag? V magnitude in the UBV systemmagphot.mag;em.opt.VB-V? B-V color in the UBV systemmagphot.color;em.opt.B;em.opt.VU-B? U-B color in the UBV systemmagphot.color;em.opt.U;em.opt.Br_UBV[1/2001]? Photometry reference numbermeta.refMKtypeSpectral typesrc.spTyper_MKtype[1/999]? Spectral type reference numbermeta.refRemarksRemarks and further cross-identifications (details in "adc.doc" or "adc.tex")meta.note
II/124A/refsAll references as a single filerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordRefNum[1/2002]? Reference numbermeta.refn_RefNum'P' for Photometry ref. ("r_UBV" in catalog), 'S' for Spectrosc. ref. ("r_MKtype in catalog)meta.noteRefText of bibliographic referencemeta.bib.bibcode
ivo://CDS.VizieR/II/1282019-06-21T18:30:00ZIIivo_managed1Photometric Data for the Bright Stars (Hauck+, 1986)II/128ivo://CDS.VizieR/II/128CDSHauck B. and Mermilliod M.Nancy Grace Roman [ADC/SSDOO]1997-12-09T15:57:19Jan-05-1996CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometryStarsReferences are given to the photometric data available for 9008 stars in the Bright Star Catalog. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?II/128CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=II/128http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=II/128GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
II/128/refsKey to the references for datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordRefNoNumber of referencemeta.refcolorColor systems includedmeta.id;photref*Referencemeta.refnoNumber of stars from referencemeta.number
II/128/catalogThe main catalogrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHRBright Star (HR, cat. <V/50>) numbermeta.id;meta.mainast[ *] Meaning of asterisk unknownmeta.noteHDHD numbermeta.idnote[ *] Asterisk indicate note in BSCmeta.noteDouble*[ D12] Double star componentmeta.notevar[ V] Indicates a variable magnitudemeta.noteVmagV magnitudemagphot.mag;em.opt.VrefReferencesmeta.ref
ivo://CDS.VizieR/II/1542019-06-21T18:30:00ZIIivo_managed1Individual UBV Observations of LSS Stars (Drilling 1989)II/154ivo://CDS.VizieR/II/154CDSDrilling J.S.C.-H. Joseph Lyu [Hughes STX/NASA] and Joseph Florsch [CDS]1997-12-09T16:00:1925-May-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometry:wide-bandUBV Photometry of Stars from "Luminous Stars in the Southern Milky Way" by J.S. Drilling, Louisiana State University Observatory, 22 July 1989. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?II/154CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=II/154http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=II/154GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
II/154/catalogUBV measurementsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordLSSLSS number (Stephenson and Sanduleak 1971)meta.id;meta.mainCompComponent identification if a double star. Where this byte is blank for the same LSS star, both components were included in the diaphragm.meta.notedateHeliocentric Julian date of observationdtime.epochVmagV magnitudemagphot.mag;em.opt.VB-VB-V color indexmagphot.color;em.opt.B;em.opt.VU-BU-B color indexmagphot.color;em.opt.U;em.opt.BAirmassAirmassobs.airMass
ivo://CDS.VizieR/II/1702019-06-21T18:30:00ZIIivo_managed1Long-term photometry of Variables I. (Manfroid+ 1991)II/170ivo://CDS.VizieR/II/170CDSManfroid J., Sterken C., Bruch A., Burger M., de Groot M., Duerbeck H.W., Duemmler R., Figer A., Hageman T., Hensberge H., Jorissen A., Madejsky R., Mandel H., Ott H.A., Reitermann A., Schulte-Ladbeck R.E., Stahl O., Steenman H., vander Linden D., ZickgraFrancois Ochsenbein [CDS]1997-12-09T16:08:5127-Nov-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometry:intermediate-bandStars:variableThis is the first catalogue of photometric data in the Stroemgren system obtained during the period October 1982 - September 1986. Full description can be found in ESO report SP 8. Since our goal is not absolute (all-sky) photometry, the observations should be used for differential photometry only. The mean values of the r.m.s. deviations of the differential measurements of comparison stars are around (from Table 5 of paper) ------------------------------------ System y b-y m1 c1 ------------------------------------ 1 0.0109 0.0088 0.0133 0.0136 4 0.0068 0.0057 0.0079 0.0118 5 0.0087 0.0070 0.0114 0.0114 6 0.0090 0.0078 0.0126 0.0132 7 0.0071 0.0033 0.0041 0.0065 ------------------------------------ http://cdsarc.u-strasbg.fr/cgi-bin/Cat?II/170CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=II/170http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=II/170GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table II/170/stars1 (The list of stars observed (10 stars missing))http://vizier.u-strasbg.fr/viz-bin/conesearch/II/170/stars1?GETtext/xml+votable18050000true46.8457031249999917.8764911249227470.028629053431811713Opticalhttp://alasky.u-strasbg.fr/footprints/cats/vizier/II/170?product=MOC&nside=512
II/170/stars1The list of stars observed (10 stars missing)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNameStar Identification, as in "catalog"meta.id;meta.mainHDHD designationmeta.idHRHR (Bright Star) designationmeta.idDMDurchmusterung (BD, CoD, CPD) designationsmeta.idName2Other designationmeta.idRAJ2000Right Ascension J2000 (hours)"h:m:s"pos.eq.ra;meta.mainDEJ2000Declination J2000 (sign)"d:m:s"pos.eq.dec;meta.mainSpSpectral classificationsrc.spType
II/170/ltpv1The ObservationsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNameStar Identification (1)meta.id;meta.mainHJD[2445243/2446704] Heliocentric Julian Datedtime.epochAirmassAirmass (sec.z)obs.airMassumagmagnitudemagphot.mag;em.opt.Uvmagmagnitudemagphot.mag;em.opt.Bbmagmagnitudemagphot.mag;em.opt.Bymagmagnitudemagphot.mag;em.opt.VT/S[14567] Telescope/system codemeta.noteR[9101] Release codemeta.code
ivo://CDS.VizieR/II/1772019-06-21T18:30:00ZIIivo_managed1Near IR Photometry of a Sample of IRAS Point Sources (Fouque+ 1992)II/177ivo://CDS.VizieR/II/177CDSFouque P., Le Bertre T., Epchtein N., Guglielmo F., Kerschbaum F.Michel Creze, Francois Ochsenbein [CDS]1997-12-09T16:09:3115-Nov-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometryStars:late-typeThe results are given for the 516 sources that we have observed from La Silla (452 in the southern hemisphere, plus 64 in the range 0 to 20deg). For each source, the IRAS name is given followed by the epoch of observation (with the convention given in Table 1), the J, H, K, L', M magnitudes that we have obtained, then three classifications based on IRAS Low Resolution Spectra (LRS), IRAS broad-band photometry (VH) and the combination of IRAS broad-band photometry with our near-infrared photometry (Val), and, finally, one association. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?II/177CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=II/177http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=II/177GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
II/177/maindata from table 2recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIRASIRAS PSC (Catalogue <II/125>) numbermeta.id;meta.mainNote[*] '*' when there is a note in table 1c of the published papermeta.noteEpochcoded according to Table 1time.epochJmag? magnitudemagphot.mag;em.IR.JHmag? magnitudemagphot.mag;em.IR.HKmag? magnitudemagphot.mag;em.IR.KL'mag? magnitudemagphot.mag;em.IR.3-4umMmag? magnitudemagphot.mag;em.IR.4-8umLRSIRAS/LRS Low resolution spectra classificationsrc.spTypeVHIRAS/VH broad band photometry classificationmeta.note;photValClassification based on IRAS/VH and authors photometry (=1987A&AS...71...39E)src.classAssocName of associated optical sourcemeta.id.assoc
ivo://CDS.VizieR/II/1882019-06-21T18:30:00ZIIivo_managed1Long-term photometry of Variables II (Sterken+, 1993)II/188ivo://CDS.VizieR/II/188CDSSterken C., Manfroid J., Anton K., Barzewski A., Bibo E., Bruch A., Burger M., Duerbeck H.W., Duemmler R., Heck A., Hensberge H., Hiesgen M., Inklaar F., Jorissen A., Juettner A., Kinkel U., Liu Zongli, Mekkaden M.V., Ng Y.K., Niarchos P., Puttmann M., SzFrancois Ochsenbein [CDS]1997-12-09T16:10:4827-Nov-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometry:intermediate-bandStars:variableThe second catalogue of the LTPV programme contains photometric data obtained during the period October 1986 - September 1990. Full description can be found in ESO reports SP 8 and 12. The data presented here have been upgraded since the printing of catalogue ESO SR 12; a major change is the use of a quite different standard, namely the ESO SAT (Stroemgren Automatic Telescope) instrumental system has been used as standard. The instrumental systems 6 and 8 can be obtained by applying the following color matrices (see ESO SR 12, page 4, Eq. (3)), inverted (b-y , y , m1 , c1): SYSTEM 6 1.05180.00000.00000.0000 0.00941.00000.00000.0000 -0.12380.00001.12060.0000 0.04260.00000.00001.0352 SYSTEM 8 1.04760.00000.00000.0000 0.03841.00000.00000.0000 -0.08770.00001.04870.0000 -0.26570.00000.00000.9732 It also very easy to go back to the same standard as in ESO SR 8 by applying the transformations given in Table 3 of ESO SR 12 (page 3). Note that the faint star C7060 is not identified so far. The mean values of the r.m.s. deviations of the differential measurements of comparison stars are around (from Table 5 of paper) ------------------------------------ System y b-y m1 c1 ------------------------------------ 6 0.0069 0.0058 0.0122 0.0129 7 0.0064 0.0030 0.0039 0.0067 8 0.0068 0.0061 0.0110 0.0097 ------------------------------------ http://cdsarc.u-strasbg.fr/cgi-bin/Cat?II/188CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=II/188http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=II/188GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table II/188/stars2 (Cross-identifications of observed stars)http://vizier.u-strasbg.fr/viz-bin/conesearch/II/188/stars2?GETtext/xml+votable18050000true65.9179687528.1856958764526060.028629053431811713Opticalhttp://alasky.u-strasbg.fr/footprints/cats/vizier/II/188?product=MOC&nside=512
II/188/ltpv2The observationsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNameStar Identification (1)meta.id;meta.mainHJD[2446704/2448166] Heliocentric Julian Datedtime.epochAirmassAirmass quantity (sec.z)obs.airMassumagu magnitudemagphot.mag;em.opt.Uvmagv magnitudemagphot.mag;em.opt.Bbmagb magnitudemagphot.mag;em.opt.Bymagy magnitudemagphot.mag;em.opt.VT/S[678] Telescope/system codemeta.noteRRelease codemeta.code
II/188/stars2Cross-identifications of observed starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNameStar Identification, as in file "ltpv2".meta.id;meta.mainHDHD designationmeta.idHRHR (Bright Star) designationmeta.idDMDurchmusterung (BD, CoD, CPD) designationsmeta.idName2Other designationmeta.idRAJ2000Right Ascension J2000 (hours)"h:m:s"pos.eq.ra;meta.mainDEJ2000Declination J2000 (sign)"d:m:s"pos.eq.dec;meta.mainSpSpectral classificationsrc.spType
ivo://CDS.VizieR/II/1932019-06-21T18:30:00ZIIivo_managed1UBV Photoelectric Cat: Data 1986-1992 (Mermilliod 1994)II/193ivo://CDS.VizieR/II/193CDSMermilliod J.-C.J.-C. Mermilliod[Lausanne/Geneve Obs.] & Gail Schneider [ADC]1997-12-09T16:12:3223-Nov-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometry:wide-bandThe previous compilation of UBV data (Mermilliod 1986a,b,c) contains the UBV photoelectric observations published between 1953 and 1986. The present supplement adds the data published between 1986 and the end of 1992 which represent 25639 new UBV data. The corresponding references were numbered in continuation of the main catalogue and go from number 1603 to 1784. See <http://obswww.unige.ch/gcpd/ph01.html> for a description of the UBV photoemtric system. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?II/193CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=II/193http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=II/193GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
II/193/catalogThe UBV data published 1986-1992recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordLIDCode number (see file codes)meta.bib.bibcoderem*[1234DS] Remark on duplicity or identification of componentsmeta.notevar[V] Remark on variabilitymeta.noteV[-1.5/20.5]? V magnitudemagphot.mag;em.opt.VB-V[-1/5]? B-V colour indexmagphot.color;em.opt.B;em.opt.VU-B[-1.5/5]? U-B colour indexmagphot.color;em.opt.U;em.opt.Bn_UBV*[S/*] Flag on the number of measurementsmeta.noteo_UBV[0/324]? Number of measurementsmeta.numberr_UBV[1603/1784] Reference key (see file refs)meta.ref
ivo://CDS.VizieR/II/194A2019-06-21T18:30:00ZIIivo_managed1Photometric study of IC 4665 (McCarthy+ 1969)II/194Aivo://CDS.VizieR/II/194ACDSMcCARTHY M.F.S.J., O'SULLIVAN S.S.J.M.-J. Wagner, James Marcout, Francois Ochsenbein [CDS]1997-12-09T16:12:3912-Jun-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frOpen_Clusters(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?II/194ACatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=II/194Ahttp://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=II/194AGETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
II/194A/table1Standard stars: photoelectric and photographic data comparedrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordVnoNumber on the plate (Vasilevskis)obs.fieldKno[1/125]? Number in Kopffmeta.idAno[1/31]? Number in Alcainometa.idBDBonner Durchmustering identificationmeta.idVpeV photoelectricmagphot.mag;em.opt.V(B-V)pe(B-V) color photoelectricmagphot.color;em.opt.B;em.opt.VVpgV photographicmagphot.mag;em.opt.V(B-V)pg(B-V) photographicmagphot.color;em.opt.B;em.opt.VNotesNotes as follows: 1 = pe data from Hogg & Kron, AJ 60, 365 2 = pe data from Johnson ApJ 119, 181 and ApJ 126, 121 3 = pe data (this paper) 4 = pe data from Coyne (priv. comm.) 5 = not used as yellow standardmeta.note
II/194A/table2General catalogue of stars observed in IC 4665 (Merging of tables 2,3,4)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordVnoNumber on the plate (Vasilevskis)obs.fieldKno[1/125]? Number in Kopffmeta.idAno[1/31]? Number in Alcainometa.idBDBonner Durchmustering identificationmeta.idB[8/15]? Photographic Bmagphot.mag;em.opt.BV[6.8/14]? photographic Vmagphot.mag;em.opt.V(B-V)[]? colormagphot.color;em.opt.B;em.opt.Ve_B[]? mean error on Bmagstat.errore_V[]? mean error on Vmagstat.errorClass[1/3]? 1=probable member, 2=Possible member, 3=Less possible membermeta.code.memberNotesNotes as follows: #1 = Less than 6 plates in B determination #2 = Less than 6 plates in V determination #3 = Identification from Kopff, Mitt. Hamburger Sternw. 8, No 52 #4 = Suspected variable #6 = Photoelectric data from Hogg & Kron, AJ 60, 365meta.note
ivo://CDS.VizieR/II/2002019-06-21T18:30:00ZIIivo_managed1Long-term photometry of Variables III (Manfroid+, 1995)II/200ivo://CDS.VizieR/II/200CDSManfroid J., Sterken C., Cunow b., de Groot M., Jorissen A., Kneer R., Krenzin R., Kruijswijk M., Naumann M., Niehues M., Schoeneich W., Sevenster M., Vos N., Vogt N.Francois Ochsenbein [CDS]1997-12-09T16:13:4027-Nov-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometry:intermediate-bandStars:variableThis is the third catalogue of photometric data in the Stroemgren system obtained during the period October 1990-January 1992 in the framework of the Long-Term Photometry of Variables (LTPV) program at the European Southern Observatory. All data have been obtained with the Danish 50-cm telescope. The mean values of the r.m.s. deviations of the differential measurements of comparison stars are around (from Table 4 of paper) ------------------------------ y b-y m1 c1 ------------------------------ 0.005 0.002 0.004 0.006 ------------------------------ http://cdsarc.u-strasbg.fr/cgi-bin/Cat?II/200CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=II/200http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=II/200GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table II/200/stars3 (The stars observed)http://vizier.u-strasbg.fr/viz-bin/conesearch/II/200/stars3?GETtext/xml+votable18050000true318.6254882812510.0104694432426080.028629053431811713http://alasky.u-strasbg.fr/footprints/cats/vizier/II/200?product=MOC&nside=512Optical
II/200/ltpv3The photometryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNameStar Identification (1)meta.id;meta.mainHJD[2448165/2448661] Heliocentric Julian Datedtime.epochAirmassAirmass quantityobs.airMassumagu magnitudemagphot.mag;em.opt.Uvmagv magnitudemagphot.mag;em.opt.Bbmagb magnitudemagphot.mag;em.opt.Bymagy magnitudemagphot.mag;em.opt.VT/S[7] Telescope/system codemeta.noteR[9502] Release codemeta.code
II/200/stars3The stars observedrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNameStar Identification, as in "ltpv3"meta.id;meta.mainn_Name[*] '*' indicates changes compared to the ESO publication (see "Historical Notes")meta.noteHDHD designationmeta.idHRHR (Bright Star) designationmeta.idDMDurchmusterung (BD, CoD, CPD) designationsmeta.idName2Other designationmeta.idRAJ2000Right Ascension J2000 (hours)"h:m:s"pos.eq.ra;meta.mainDEJ2000Declination J2000 (sign)"d:m:s"pos.eq.dec;meta.mainSpSpectral classificationsrc.spType
ivo://CDS.VizieR/II/2022019-06-21T18:30:00ZIIivo_managed1Long-term photometry of Variables IV (Sterken+, 1995)II/202ivo://CDS.VizieR/II/202CDSSterken C., Manfroid J., Beele D., de Koff S., Eggenkamp I.M.M.G., Goecking K., Jorissen A., Kaufer A., Kuss C., Schoenmakers A.P., Still J.M., van Loon J., Vink J., Vrielmann S., Waelde E.Francois Ochsenbein [CDS]1997-12-09T16:14:0121-Oct-1996CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometry:intermediate-bandStars:variableThis is the fourth catalogue of photometric data in the Stroemgren system obtained during the period June 18, 1992 - August 23, 1994 in the framework of the Long-Term Photometry of Variables (LTPV) program at the European Southern Observatory. Since our goal is not absolute (all-sky) photometry, the observations should be used for differential photometry only. The mean values of the r.m.s. deviations of the differential measurements of comparison stars are around (from Table 3 of paper) ------------------------------ y b-y m1 c1 ------------------------------ 0.005 0.002 0.004 0.007 ------------------------------ http://cdsarc.u-strasbg.fr/cgi-bin/Cat?II/202CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=II/202http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=II/202GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table II/202/stars4 (The list of stars observed)http://vizier.u-strasbg.fr/viz-bin/conesearch/II/202/stars4?GETtext/xml+votable18050000true318.6254882812510.0104694432426080.028629053431811713Opticalhttp://alasky.u-strasbg.fr/footprints/cats/vizier/II/202?product=MOC&nside=512
II/202/stars4The list of stars observedrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNameStar Identification, as in file "ltpv4".meta.id;meta.mainHDHD designationmeta.idHRHR (Bright Star) designationmeta.idDMDurchmusterung (BD, CoD, CPD) designationsmeta.idName2Other designationmeta.idRAJ2000Right Ascension J2000 (hours)"h:m:s"pos.eq.ra;meta.mainDEJ2000Declination J2000 (sign)"d:m:s"pos.eq.dec;meta.mainSpSpectral classificationsrc.spType
II/202/ltpv4*The observationsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNameStar Identification (1)meta.id;meta.mainHJD[2448791/2449596] Heliocentric Julian Datedtime.epochAirmassAirmass quantity (sec.z)obs.airMassymagStroemgren's y magnitudemagphot.mag;em.opt.Vb-yStroemgren's b-y colourmagphot.color;em.opt.B;em.opt.Vm1Stroemgren's m1 ((v-b)-(b-y)) colourmagphot.colorc1Stroemgren's c1 ((u-v)-(v-b)) colourmagphot.colorT/S[N] Telescope/system code ("N" is the "natural" system")meta.note
ivo://CDS.VizieR/II/2082019-06-21T18:30:00ZIIivo_managed1BVRI CCD photometry in the field of M 31 (Magnier+ 1992)II/208ivo://CDS.VizieR/II/208CDSMagnier E.A., Lewin W.H.G., van Paradijs J., Hasinger G., Jain A., Pietsch W., Truemper J.Francois Ochsenbein [CDS]1997-12-09T16:15:4906-Sep-1996CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometryStarsDeep BVRI CCD photometry was performed on a 1 square degree region of M31. The observations were made between September 12 and September 27, 1990, using the McGraw-Hill 1.3m telescope at the Michigan-Dartmouth-MIT (MDM) observatory at Kitt Peak. The catalogue has typical completion limits of 22.3Bmag, 22.2Vmag, 22.2Rmag and 20.9Imag. Photometric accuracy is about 2% at Vmag=19. The final astrometric calibrations take into account the systematic error discovered in the Berkhuijsen etal (1987) catalog (Magnier etal 1993). They are in the J2000 system and are eventually tied to the HST Guide Star Catalog. The final photometric calibrations are tied via the NGC 206 region to photometry taken at the Michigan-Dartmouth-MIT (MDM) 1.3m in September and October 1993. These are tied to the Landolt (1992) system of standard stars, and are in the Johnson-Kron-Cousins system (BVRcIc). http://cdsarc.u-strasbg.fr/cgi-bin/Cat?II/208CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=II/208http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=II/208GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table II/208/bv (Stars with both B and V photometry)http://vizier.u-strasbg.fr/viz-bin/conesearch/II/208/bv?GETtext/xml+votable18050000true9.975585937540.057397202965110.028629053431811713Opticalhttp://alasky.u-strasbg.fr/footprints/cats/vizier/II/208?product=MOC&nside=512
II/208/bvStars with both B and V photometryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordSeq[1,485425]+ Sequence numbermeta.id;meta.mainRAJ2000Right ascension (J2000)degpos.eq.ra;meta.maine_RAdegScatter for the star, if multiple measurementsdegstat.errorDEJ2000Declination (J2000)degpos.eq.dec;meta.maine_DEdegScatter if multiple measurementsdegstat.errorBmag? B magnitudemagphot.mag;em.opt.Be_Bmag? Mean error on Bmagmagstat.erroro_Bmag[-5,7] Number of detection in B images (2)meta.numbertBmag[0-57] DoPHOT type for each detection (1)src.classVmag? V magnitudemagphot.mag;em.opt.Ve_Vmag? Mean error on Vmagmagstat.erroro_Vmag[-6,7] Number of detection in V images (2)meta.numbertVmag[0-57] DoPHOT type for each detection (1)src.classRmag? R magnitude (Cousins)magphot.mag;em.opt.Re_Rmag? Mean error on Rmagmagstat.erroro_Rmag[-5,6] Number of detection in R images (2)meta.numbertRmag[0-57] DoPHOT type for each detection (1)src.classImag? I magnitude (Cousins)magphot.mag;em.opt.Ie_Imag? Mean error on Imagmagstat.erroro_Imag[-5,6] Number of detection in I images (2)meta.numbertImag[0-57] DoPHOT type for each detection (1)src.class
ivo://CDS.VizieR/III/1472019-06-21T18:30:00ZIIIivo_managed1Studies of LMC stellar content (Rousseau+ 1978)III/147ivo://CDS.VizieR/III/147CDSRousseau J., Martin N., Prevot L., Rebeirot E., Robin A., Brunet J.P.Francois Ochsenbein [CDS]1997-12-09T16:35:1301-Sep-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frThis is an updated version of the original catalogue. New UBV photoelectric measurements were added from Isserstedt (1979, 1982), and Feitzinger and Isserstedt (1983). The remarks and origins of photoelectric photoelectric magnitudes are not included in this electronic version. Photoelectric data are obtained by averaging observational values made at 100 and more cm instruments (with weight=2) with ones made at 60 and less cm instruments (with weight=1). http://cdsarc.u-strasbg.fr/cgi-bin/Cat?III/147CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=III/147http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=III/147GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table III/147/catalog (The catalogue)http://vizier.u-strasbg.fr/viz-bin/conesearch/III/147/catalog?GETtext/xml+votable18050000true82.94228356336262-71.716913242329620.028629053431811713http://alasky.u-strasbg.fr/footprints/cats/vizier/III/147?product=MOC&nside=512Optical
III/147/catalogThe cataloguerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNameIdentification (1)meta.id;meta.mainBchartNumber of B chart Hodge and Wright (1967) (2)meta.numberRA1975Right Ascension 1975 (hours)"h:m:s"pos.eq.ra;meta.mainDE1975Declination 1975 (sign)"d:m:s"pos.eq.dec;meta.mainSpTypeSpectral type (3)src.spTyper_SpTypeOrigin of the spectral type (4)meta.refVmag? V photoelectric magnitudemagphot.mag;em.opt.Vu_VmagUncertainty flag (:) on Vmagmeta.code.errorB-V? photoelectric colour indexmagphot.color;em.opt.B;em.opt.Vu_B-VUncertainty flag (:) on B-Vmeta.code.errorU-B? photoelectric colour indexmagphot.color;em.opt.U;em.opt.Bu_U-BUncertainty flag (:) on U-Bmeta.code.errorObs? Number of photoelectric measurementsmeta.numberPmag? V photographic magnitude (5)magphot.mag;em.opt.Vu_PmagUncertainty flag (:) on Pmag (5)meta.code.erroro_Pmag? Number of plates used for Pmag determinationmeta.number
ivo://CDS.VizieR/III/1862019-06-21T18:30:00ZIIIivo_managed1Energy distribution in stars at 320-760 nm (Knyazeva+, 1996)III/186ivo://CDS.VizieR/III/186CDSKnyazeva L.N., Kharitonov A.V.Veta Avedisova [INASAN]1997-12-09T16:40:4230-Dec-1996CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frStarsSpectrophotometryThe intrinsic energy distribution for 41 spectral subclasses in the range of wavelengths of 320-760 nm are derived in the following way: (1) The sources of the spectrophotometric data were taken from three catalogues published in FSU (Kharitonov et al. 1988, Glushneva, ed., 1982, Alekseeva et al. 1992), containing energy distributions of about 2000 stars of different spectral types. (2) MK spectral classes were taken from the Bright Star Catalogue (Hoffleit 1982; hereafter BSC). The paper by Gray and Garrison (1987) was took into account to examine the influence of errors in spectral classification. (3) The quality of stars selected for each subclass was estimated by comparison of the observed and synthetic (U-B) and (B-V) color indices calculated for our energy distributions. The results have been published by Knyazeva and Kharitonov (1993, 1994a, 1994b, 1996a, 1996b) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?III/186CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=III/186http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=III/186GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
III/186/tableIntrinsic energy distribution for spectral subclasses (relative to maximum)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordLambda[3225/7575] Spectral line wavelengthnmem.wlE(B5V)Intrinsic energy for B5Vphot.flux.density;em.optE(B7V)Intrinsic energy for B7Vphot.flux.density;em.optE(B8V)Intrinsic energy for B8Vphot.flux.density;em.optE(B9V)Intrinsic energy for B9Vphot.flux.density;em.optE(B9.5V)Intrinsic energy for B9.5Vphot.flux.density;em.optE(A0V)Intrinsic energy for A0Vphot.flux.density;em.optE(A1V)Intrinsic energy for A1Vphot.flux.density;em.optE(A2V)Intrinsic energy for A2Vphot.flux.density;em.optE(A3V)Intrinsic energy for A3Vphot.flux.density;em.optE(A4V)Intrinsic energy for A4Vphot.flux.density;em.optE(A5V)Intrinsic energy for A5Vphot.flux.density;em.optE(A7V)Intrinsic energy for A7Vphot.flux.density;em.optE(A3IV)Intrinsic energy for A3IVphot.flux.density;em.optE(A7IV)Intrinsic energy for A7IVphot.flux.density;em.optE(F0V)Intrinsic energy for F0Vphot.flux.density;em.optE(F5V)Intrinsic energy for F5Vphot.flux.density;em.optE(F6V)Intrinsic energy for F6Vphot.flux.density;em.optE(F7V)Intrinsic energy for F7Vphot.flux.density;em.optE(F8V)Intrinsic energy for F8Vphot.flux.density;em.optE(F0IV)Intrinsic energy for F0IVphot.flux.density;em.optE(F2IV)Intrinsic energy for F2IVphot.flux.density;em.optE(F5IV)Intrinsic energy for F5IVphot.flux.density;em.optE(G0V)Intrinsic energy for G0Vphot.flux.density;em.optE(G2V)Intrinsic energy for G2Vphot.flux.density;em.optE(G5V)Intrinsic energy for G5Vphot.flux.density;em.optE(G8V)Intrinsic energy for G8Vphot.flux.density;em.optE(G7III)Intrinsic energy for G7IIIphot.flux.density;em.optE(G8III)Intrinsic energy for G8IIIphot.flux.density;em.optE(G9III)Intrinsic energy for G9IIIphot.flux.density;em.optE(K0III)Intrinsic energy for K0IIIphot.flux.density;em.optE(K1III)Intrinsic energy for K1IIIphot.flux.density;em.optE(K2III)Intrinsic energy for K2IIIphot.flux.density;em.optE(K3III)Intrinsic energy for K3IIIphot.flux.density;em.optE(K4III)Intrinsic energy for K4IIIphot.flux.density;em.optE(K5III)Intrinsic energy for K5IIIphot.flux.density;em.optE(M0III)Intrinsic energy for M0IIIphot.flux.density;em.optE(M1III)Intrinsic energy for M1IIIphot.flux.density;em.optE(M2III)Intrinsic energy for M2IIIphot.flux.density;em.optE(M3III)Intrinsic energy for M3IIIphot.flux.density;em.optE(M4III)Intrinsic energy for M4IIIphot.flux.density;em.optE(M5III)Intrinsic energy for M5IIIphot.flux.density;em.opt
ivo://CDS.VizieR/IV/122019-06-21T18:30:00ZIVivo_managed1SAO-HD-GC-DM Cross Index (ADC 1983) (Roman+ 1983)IV/12ivo://CDS.VizieR/IV/12CDSRoman N.G., Warren Jr. W.H., Schofield Jr. N.J.Gail L. Schneider [SSDOO/ADC], Francois Ochsenbein [CDS]1997-12-09T16:56:2613-May-1996CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frStarsThe catalog is an updated, corrected, and extended version of a table of correspondences originally prepared by Morin (1973). The individual data corrections, additions, and changes included in the new version number 11398, with 8600 data records having at least one change. In addition to the correction of all errors found since preparation of the original catalog, most of which resulted from misidentifications and omissions of components in multiple-star systems and missing Durchmusterung numbers (the common identifier) in the SAO Catalog, component identifications from the Index Catalogue of Visual Double Stars (IDS) have been appended to all multiple SAO stars having the same DM numbers, and lowercase identifications for supplemental (footnoted) BD stars have been added. Stars deleted (duplicate entries) in the SAO Catalog have been appended with a "D" and their data removed, although the records have been kept (with SAO number only) in order not to change the number of SAO stars. The data include SAO number, HD number, HD multiplicity code, GC number, DM identification code (BD, CD, CP), and number. There are fewer objects than records because of the deleted entries appended with a "D" as described above (35 stars deleted). http://cdsarc.u-strasbg.fr/cgi-bin/Cat?IV/12CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=IV/12http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=IV/12GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table IV/12/index (The SAO-HD-GC-DM Cross Index)http://vizier.u-strasbg.fr/viz-bin/conesearch/IV/12/index?GETtext/xml+votable18050000true45.04394531250.242463332287780080.028629053431811713http://alasky.u-strasbg.fr/footprints/cats/vizier/IV/12?product=MOC&nside=512Optical
IV/12/indexThe SAO-HD-GC-DM Cross IndexrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordSAO[1/258997]+ SAO Catalog numbermeta.id;meta.mainRAJ2000Hours RA, equinox J2000"h:m:s"pos.eq.ra;meta.mainDEJ2000Sign Dec, equinox J2000"d:m:s"pos.eq.dec;meta.mainDM*Durchmusterung catalog IDmeta.idHD[1/359083]? Henry Draper Catalog (HD) numbermeta.idm_HD*[0129] HD number code (see comment)meta.code.multipGC[1/33342]? Boss General Catalog (GC) numbermeta.id
ivo://CDS.VizieR/IX/132019-06-21T18:30:00ZIXivo_managed1The 2E Catalogue (Harris+ 1994)IX/13ivo://CDS.VizieR/IX/13CDSHarris D.E., Forman W, Gioa I.M., Hale J.A., Harnden Jr. F.R., Jones C., Karakashian T., Maccacaro T., McSweeney J.D., Primnini F.A., Schwarz J., Tananbaum H.D., Thurman J.Jean-Marie Hameury [Strasbourg]1997-12-09T17:10:351996-Oct-25CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frThis catalog contains sources from EINSTEIN IPC (Imaging Proportional counter aboard the EINSTEIN (HEAO 2) satellite, in orbit between November 1978 and April 1981) detected during pointed observations. Note that a single source may have more than one entry in the catalog. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?IX/13CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=IX/13http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=IX/13GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table IX/13/2e (The catalogue)http://vizier.u-strasbg.fr/viz-bin/conesearch/IX/13/2e?GETtext/xml+votable18050000true45.285644531249993.50857471197746570.028629053431811713Einsteinhttp://alasky.u-strasbg.fr/footprints/cats/vizier/IX/13?product=MOC&nside=512X-ray
IX/13/2eThe cataloguerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordCATNUM[1/4809]+= Catalogue number of the source (1)meta.id;meta.mainSEQNUMSequence number for the observationmeta.idFLDNUMField number of the sourceobs.fieldRA1950Right ascension 1950 (hours)"h:m:s"pos.eq.ra;meta.mainDE1950Declination 1950 (sign)"d:m:s"pos.eq.dec;meta.mainPosErrPositional error (arcsec)arcsecstat.errorCrateCorrected count ratect/sphot.count;em.X-raye_CrateError on the count ratect/sstat.errorLivTimeLive time (in seconds, at the field center)stime.duration;obs.exposureNetCountNet counts in the detect cellphot.count;em.X-rayBkgCountBackground counts in the detect cellinstr.backgroundS/NSignal to noise ratio for the detectionstat.snrSizCorSize correction factor (2)arith.factorRECodeRibs and edges code (3)meta.codeOffAxisDist. between source & field center (arcmin)arcminpos.angDistanceSrcFlag[AaHLEI ] Source flags (4)meta.codeRefFlagReference and identification flag (5)meta.ref
ivo://CDS.VizieR/J/A+A/265/322019-06-21T18:30:00ZJ.A_Aivo_managed1Radial structure of the galactic disc (Robin+ 1992)J/A+A/265/32ivo://CDS.VizieR/J/A+A/265/32CDSRobin A.C., Creze M., Mohan V.[CDS]1997-12-09T17:11:3802-Mar-1993CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometry(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/265/32CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/265/32http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/265/32GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table J/A+A/265/32/fields (Positions and UBV, fields 1 to 4 (V <= 25))http://vizier.u-strasbg.fr/viz-bin/conesearch/J/A+A/265/32/fields?GETtext/xml+votable18050000true89.0112304687530.604870563949020.028629053431811713Opticalhttp://alasky.u-strasbg.fr/footprints/cats/vizier/J/A+A/265/32?product=MOC&nside=512
J/A+A/265/32/fieldsPositions and UBV, fields 1 to 4 (V <= 25)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordField[1/4] Field numberobs.fieldNumberRunning number in fieldmeta.id.part;meta.mainRAJ2000J2000 right ascension"h:m:s"pos.eq.ra;meta.mainDEJ2000J2000 declination"d:m:s"pos.eq.dec;meta.mainVmagV magnitude transformed to Johnson systemmagphot.mag;em.opt.VB-V? B-V color index (Johnson system)magphot.color;em.opt.B;em.opt.VU-B? U-B color index (Johnson system)magphot.color;em.opt.U;em.opt.B
ivo://CDS.VizieR/II/852019-06-21T18:30:00ZIIivo_managed1Absolute Calibration of Stellar Spectrophotometry (Johnson 1980)II/85ivo://CDS.VizieR/II/85CDSJohnson H.L.Francois Ochsenbein [CDS]1997-12-09T17:12:3029-Apr-1997CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frSpectrophotometryThe catalog contains the absolute fluxes for 16 stars published in Tables 1 and 2 of Johnson (1980). The absolute calibrations were accomplished by combining the 13-color photometry calibrations of Johnson and Mitchell (1975) with spectra obtained with a Michelson spectrophotometer and covering the wavelength range 4000 to 10300 Angstroms (Johnson 1977). The agreement between the absolute calibration and another recent one based upon data for alpha Lyr and 109 Vir by Tug et al. (1977) is shown (Johnson 1980) to be quite good. The catalog includes star name, cross identifications to the numbering systems of the Bright Star Catalogue and The Henry Draper Catalogue and arrays of fluxes having the same number of elements for each of the 16 stars. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?II/85CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=II/85http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=II/85GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
II/85/catalogThe Absolute fluxes of 16 starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordlambdaWavelengthnmem.wlF01Flux for HR 7906 = HD 196867 = alf DelmW/m2/Hzphot.fluxF02Flux for HR 5685 = HD 135742 = bet LibmW/m2/Hzphot.fluxF03Flux for HR 4662 = HD 106625 = gam CrvmW/m2/Hzphot.fluxF04Flux for HR 6629 = HD 161868 = gam OphmW/m2/Hzphot.fluxF05Flux for HR 4942 = HD 113791 = xi2 CetmW/m2/Hzphot.fluxF06Flux for HR 7235 = HD 177724 = zet AqlmW/m2/Hzphot.fluxF07Flux for HR 875 = HD 18331mW/m2/Hzphot.fluxF08Flux for HR 3314 = HD 71155mW/m2/Hzphot.fluxF09Flux for HR 2491 = HD 48915 = alf CMamW/m2/Hzphot.fluxF10Flux for HR 7001 = HD 172167 = alf LyrmW/m2/Hzphot.fluxF11Flux for HR 8781 = HD 218045 = alf PegmW/m2/Hzphot.fluxF12Flux for HR 4534 = HD 102647 = bet LeomW/m2/Hzphot.fluxF13Flux for HR 1855 = HD 36512 = ups OrimW/m2/Hzphot.fluxF14Flux for HR 8622 = HD 214680 = 10 LacmW/m2/Hzphot.fluxF15Flux for HR 5511 = HD 130109 = 109 VirmW/m2/Hzphot.fluxF16Flux for HR 8634 = HD 214923 = zet PegmW/m2/Hzphot.flux
ivo://CDS.VizieR/J/A+A/271/5152019-06-21T18:30:00ZJ.A_Aivo_managed1Atmospheric parameters of A and F stars I. (Smalley+ 1993)J/A+A/271/515ivo://CDS.VizieR/J/A+A/271/515CDSSmalley B., Dworetsky M.M.09-Feb-1991997-12-09T17:12:3509-Feb-1993CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frSpectroscopy(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/271/515CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/271/515http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/271/515GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/271/515/gammaH gamma profilesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHRnumbermeta.id;meta.mainHDnumbermeta.idR1Residual flux at 1 angstrom from line corestat.fit.residualR2Residual flux at 2 angstroms from line corestat.fit.residualR4Residual flux at 4 angstroms from line corestat.fit.residualR6Residual flux at 6 angstroms from line corestat.fit.residualR8Residual flux at 8 angstroms from line corestat.fit.residualR10Residual flux at 10 angstroms from line corestat.fit.residualR15Residual flux at 15 angstroms from line corestat.fit.residualR20Residual flux at 20 angstroms from line corestat.fit.residualR25Residual flux at 25 angstroms from line corestat.fit.residualR30Residual flux at 30 angstroms from line corestat.fit.residualR35Residual flux at 35 angstroms from line corestat.fit.residualR40Residual flux at 40 angstroms from line corestat.fit.residual
J/A+A/271/515/betaH beta profilesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHRnumbermeta.id;meta.mainHDnumbermeta.idR1Residual flux at 1 angstrom from line corestat.fit.residualR2Residual flux at 2 angstroms from line corestat.fit.residualR4Residual flux at 4 angstroms from line corestat.fit.residualR6Residual flux at 6 angstroms from line corestat.fit.residualR8Residual flux at 8 angstroms from line corestat.fit.residualR10Residual flux at 10 angstroms from line corestat.fit.residualR15Residual flux at 15 angstroms from line corestat.fit.residualR20Residual flux at 20 angstroms from line corestat.fit.residualR25Residual flux at 25 angstroms from line corestat.fit.residualR30Residual flux at 30 angstroms from line corestat.fit.residualR35Residual flux at 35 angstroms from line corestat.fit.residualR40Residual flux at 40 angstroms from line corestat.fit.residual
ivo://CDS.VizieR/J/A+A/275/4842019-06-21T18:30:00ZJ.A_Aivo_managed11990-1992 Photometry of UU Her (Zsoldos+ 1993)J/A+A/275/484ivo://CDS.VizieR/J/A+A/275/484CDSZsoldos E., Fernie J.D., Ferro A. Arellano, Seager S.[CDS]1997-12-09T17:13:1218-May-1993CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometry:wide-bandPhotometry:intermediate-bandStars:variable(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/275/484CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/275/484http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/275/484GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOpticalInfrared
J/A+A/275/484/table3buvbybeta photometry of UU HerrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordJuliandate-2440000dtime.epochVmagnitudemagphot.mag;em.opt.Vu_VUncertainty flag (:) on Vmeta.code.error(b-y)colourmagphot.color;em.opt.B;em.opt.Vu_(b-y)Uncertainty flag (:) on (b-y)meta.code.errorm1colourmagphot.coloru_m1Uncertainty flag (:) on m1meta.code.errorc1colourmagphot.coloru_c1Uncertainty flag (:) on c1meta.code.errorbetamagnitudemagphot.color;em.line.Hbetau_betaUncertainty flag (:) on betameta.code.error
J/A+A/275/484/table1V and (b-y) photometry of UU HerrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordJDJulian day-2440000dtime.epochVmagmagnitudemagphot.mag;em.opt.B(b-y)? colourmagphot.color;em.opt.B;em.opt.V
J/A+A/275/484/table3aBVRI photometry of UU HerrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordJuliandate-2440000dtime.epochVmagnitudemagphot.mag;em.opt.V(B-V)colourmagphot.color;em.opt.B;em.opt.V(V-R)colourmagphot.color;em.opt.V;em.opt.R(V-I)? colourmagphot.color;em.opt.V;em.opt.I
J/A+A/275/484/table2UBV photometry of UU HerrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordJuliandate-2440000dtime.epochVmagnitudemagphot.mag;em.opt.Vu_VUncertainty flag (:) on Vmeta.code.error(B-V)colourmagphot.color;em.opt.B;em.opt.Vu_(B-V)Uncertainty flag (:) on (B-V)meta.code.error(U-B)? colourmagphot.color;em.opt.U;em.opt.Bu_(U-B)Uncertainty flag (:) on (U-B)meta.code.error
ivo://CDS.VizieR/J/A+A/275/5492019-06-21T18:30:00ZJ.A_Aivo_managed1Interstellar extinction curves (Jenniskens+ 1993)J/A+A/275/549ivo://CDS.VizieR/J/A+A/275/549CDSJenniskens P., Greenberg J.M.Patricia Bauer [CDS]1997-12-09T17:13:2310-Sep-1993CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometryExtinctionThe data are a decomposition of the extinction curves published by Aiello S., Barsella B., Chlewicki G., Greenberg J.M., Patriarchi P., and Perinotto M. (1988A&AS...73..195A) in the parameter scheme of Fitzpatrick E.L. and Massa D. (1988ApJ...328..734F). Each extinction curve k(x) = (A(lambda)-A(V))/(A(B)-A(V)) is given by: k(x) = c1 + c2*x + c3* D(x,x0,y) + c4*F(x) Where x = 1/wavelength (in inverse micron), D is a Drude profile: D(x,x0,y) = x^2^/((x^2^-x0^2^)^2^ + y^2^x^2^) and F is a polynomial of order 3: F(x) = 0.05392(x-5.9)^2^ + 0.0564(x-5.9)^3^ for 5.9<x<8.0 F(x) = 0 for x<5.9 In this scheme the parameters have the following meaning: c1: related directly to c2 because of normalisation k(x) c2: slope of the linear rise ( mag/E(B-V) ) y: width of the bump (inverse micron) c3: c3/y^2^ is bump height, pi*c3/(2.*y) is bump area x0: position of the bump (inverse micron) c4: amount of FUV non-linear rise contribution: at 8 mu^-1^: 2.9c4 (mag/E(B-V)) | * ^ | *2.9c4 |^** k(x)| c3/y^2* * * .. v | *< y >**.. |v * .. * * |*.. c2 1 | * 0 |* |^* |Rv * |v____________________________|_____________________________ V B x0 5.9 8.0 x=1/wavelength (1/micron) Values of Rv, the ratio of total to selective extinction, can be found in Aiello et al. (1988A&AS...73..195A). http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/275/549CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/275/549http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/275/549GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapUV
J/A+A/275/549/tableExtinction coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordstarnameDesignation of star.meta.id;meta.maink(U)? Extinction in U bandobs.atmos.extinctionc1Coefficient (see text)stat.fit.paramc2Coefficient (see text)umstat.paramc3Coefficient (see text)stat.fit.paramc4Coefficient (see text)stat.fit.paramyWidth of the bumpum-1phys.absorption.coeffx0Position of the bumpum-1phys.absorption.coeffchisqIndication of the deviation between fitted curve and actual datastat.fit.paramQQuality indication of the data (1)meta.code.qualIPSC[0/2] IRAS point source classification (2)src.classTYPEEnvironment characterisation from IRAS Skyflux maps (3)src.morph.type
ivo://CDS.VizieR/J/A+A/276/1422019-06-21T18:30:00ZJ.A_Aivo_managed1Compositional differences among the A-type stars (Hill+ 1993)J/A+A/276/142ivo://CDS.VizieR/J/A+A/276/142CDSHill G.M., Landstreet J.D.[CDS]1997-12-09T17:13:4614-Apr-1993CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frAbundances(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/276/142CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/276/142http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/276/142GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/276/142/table2Line list for spectrum synthesisrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIdElement identificationphys.atmol.elementlambdaWavelength (A)0.1nmem.wllog.gflog gfphys.atmol.wOscStrengthRefReference (1)meta.ref
ivo://CDS.VizieR/J/A+A/276/3452019-06-21T18:30:00ZJ.A_Aivo_managed1Photometry of variable LQ Hya (Jestu 1993)J/A+A/276/345ivo://CDS.VizieR/J/A+A/276/345CDSJestu L.Patricia Bauer [CDS]1997-12-09T17:14:015-Oct-1993CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometry:wide-band(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/276/345CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/276/345http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/276/345GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/276/345/table4ResultsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordYearYear of observationtime.epochP(phot)? Photometric rotation period (1)dtime.periode_P(phot)? rms uncertainty on P(phot)dstat.errorPhi(m,1)Phase of primary minimum (2)time.phasee_Phi(m,1)rms uncertainty on Phi(m,1)stat.errorPhi(m,2)? Phase of secondary minimum (2)time.phasee_Phi(m,2)? rms uncertainty on Phi(m,2)stat.errorM(V)Mean magnitude in V (3)magphot.mag;em.opt.Ve_M(V)rms uncertainty on M(V)magstat.errorM(B)? Mean magnitude in B (3)magphys.magAbs;em.opte_M(B)? rms uncertainty on M(V)magstat.errorA(V)Amplitude of rotational modulation in V (3)magsrc.var.amplitudee_A(V)rms uncertainty on A(V)magstat.errorA(B)?Amplitude of rotational modulation in B (3)magsrc.var.amplitudee_A(B)? rms uncertainty on A(B)magstat.errorSETDivision into subsets of the observing timemeta.id
J/A+A/276/345/table3LQ Hya new APT photometryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHJD-2440000Observing time: HJD-2440000dtime.epochBmag? B magnitudemagphot.mag;em.opt.BVmag? V magnitudemagphot.mag;em.opt.VSETDivision into subsets of the observing timemeta.id
J/A+A/276/345/table1LQ Hya Johnson BV photometry (APT), Boyd et al., 1990recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHJD-2440000Observing time: HJD-2440000dtime.epochBmag? B magnitudemagphot.mag;em.opt.BVmag? V magnitudemagphot.mag;em.opt.VSETDivision into subsets of the observing timemeta.id
ivo://CDS.VizieR/J/A+A/276/3892019-06-21T18:30:00ZJ.A_Aivo_managed1The spectrum of FG Sge in 1992 (Kipper+, 1993)J/A+A/276/389ivo://CDS.VizieR/J/A+A/276/389CDSKipper T., Kipper M.Patricia Bauer [CDS]1997-12-09T17:14:141996-Jan-10CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frAbundancesWavelength measurements and line identifications from the 0.14A/pixel echelle spectra of FG Sge secured two weeks before the drastic dimming of the star in 1992 are presented. The abundances of 18 elements are derived. These abundances have not changed from 1986. The main features of the chemical composition of FG Sge atmosphere are the depletion of iron-group elements and the marked overabundances (up to 3 dex) of s-process elements. First time in the observational history of FG Sge C_2_ Swan bands are identified in its spectrum. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/276/389CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/276/389http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/276/389GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/276/389/table2Line identifications in FG SgerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordLamObsMeasured wavelength0.1nmem.wlRcEye estimate of the residual intensity R_c_ multiplied by 10phot.count;em.optLam[]? Identification wavelength0.1nmem.wlNameName of the line identifiedmeta.id
ivo://CDS.VizieR/J/A+A/278/362019-06-21T18:30:00ZJ.A_Aivo_managed1M 31 new OB associations (Magnier+ 1993)J/A+A/278/36ivo://CDS.VizieR/J/A+A/278/36CDSMagnier E.A., Battinelli P., Lewin W.H.G., Haiman Z., Van Paradijs J., Hasinger G., Pietsch W., Supper R., Trumper J.James Marcout, Patricia Bauer [CDS]1997-12-09T17:14:2526-Sep-1997CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frAssociationsPositional_DataA new identification of OB associations in M 31 has been performed using the Path Linkage Criterion technique of Battinelli (1991A&A...244...69B). We found 174 associations with a very small contamination (<5%) by random clumps stars. The expected total number and average size of OB associations in the region of M 31 covered by our data set (Magnier et al., 1992, Cat. <II/208>) are ~280 and ~90pc, respectively. M 31 associations therefore have sizes similar to those of OB associations observed in nearby galaxies, so that we can consider them to be classical OB associations. This list of OB associations will be used for the study of the spatial distribution of OB associations and their correlation with other objects. Taking into account the fact that we do not cover the entire disk of M 31, we extrapolate a total number of associations in M 31 of ~420. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/278/36CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/278/36http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/278/36GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table J/A+A/278/36/table1 (Associations in M 31)http://vizier.u-strasbg.fr/viz-bin/conesearch/J/A+A/278/36/table1?GETtext/xml+votable18050000true10.10742187500000240.497439252771190.028629053431811713http://alasky.u-strasbg.fr/footprints/cats/vizier/J/A+A/278/36?product=MOC&nside=512Optical
J/A+A/278/36/table1Associations in M 31recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordMLB93OB association numbermeta.id;meta.mainRAJ2000Right ascension (J2000.0)degpos.eq.ra;meta.mainDEJ2000Declination (J2000.0)degpos.eq.dec;meta.mainDiamClump diameterpcphys.size.diameterNStarNumber of starsmeta.number
ivo://CDS.VizieR/J/A+A/278/3792019-06-21T18:30:00ZJ.A_Aivo_managed1X-ray Emission from Abell Clusters of Galaxies (Briel+ 1993)J/A+A/278/379ivo://CDS.VizieR/J/A+A/278/379CDSBriel U.G., Henry J.P.Patricia Bauer [CDS]1997-12-09T17:14:3722-Dec-1993CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frClusters_of_galaxiesThe results of ROSAT All-Sky Survey (RASS, see cat. <IX/10>) have been used to investigate the X-ray properties of a complete sample of Abell clusters within a 561 square degree region at high galactic latitude; the mean redshift of the sample is 0.17. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/278/379CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/278/379http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/278/379GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table J/A+A/278/379/table1 (Summary of the characteristics and X-ray results of the deep cluster sample)http://vizier.u-strasbg.fr/viz-bin/conesearch/J/A+A/278/379/table1?GETtext/xml+votable18050000true178.9942321557317757.89899240623980.028629053431811713X-rayhttp://alasky.u-strasbg.fr/footprints/cats/vizier/J/A+A/278/379?product=MOC&nside=512
J/A+A/278/379/table1Summary of the characteristics and X-ray results of the deep cluster samplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordAbellAbell Numbermeta.id;meta.mainRA1950Right Ascension (1950) (1)"h:m:s"pos.eq.ra;meta.mainDE1950Declination sign (1)"d:m:s"pos.eq.dec;meta.mainzRedshiftsrc.redshiftRich.Abell's richnesssrc.class.richnessACOACO's galaxy countsmeta.numberN(HI)Galactic neutral hydrogen column density10+21/cm2phys.columnDensityFCCCFraction of cluster counts collectedinstr.paramExpROSAT-All-Sky-Survey exposure timestime.duration;obs.exposureNCRNet counting ratect/ksphot.count;em.X-raye_NCR1-sigma error of the counting ratect/ksstat.errorl_XFluxlimit flag on X-ray fluxmeta.code.errorXFluxX-ray flux in 0.5-2.5 keV (observed frame)10-16W/m2phot.flux;em.X-rayl_XLumlimit flag on X-ray luminositymeta.code.errorXLumX-ray luminosity in 0.5-2.5 keV (rest frame) for H_o = 50 km/s/Mpc and q_o = 0.5 (unit 10+44 erg/s)10+37Wphys.luminosity;em.X-ray
ivo://CDS.VizieR/J/A+A/281/152019-06-21T18:30:00ZJ.A_Aivo_managed1Asymmetries in radio source structures (Rys 1994)J/A+A/281/15ivo://CDS.VizieR/J/A+A/281/15CDSRYS S.Patricia Bauer [CDS]1997-12-09T17:15:1712-Oct-1993CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frGalaxies(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/281/15CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/281/15http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/281/15GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapRadio
J/A+A/281/15/table1The data samplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNameIAU source namemeta.id;meta.mainIdoptical identificationmeta.id.crossV[]? optical magnitudemagphot.mag;em.opt.VFtottotal flux at 1.4 GHz (in radio map)Jyphot.flux.density;em.radio.750-1500MHzalfspectral index (power law: freq**(-alf))spect.indexLASlargest angular sizearcsecphys.angSize;srcMCnumber of map componentsmeta.number
J/A+A/281/15/table2The best fitting parameters for the modelsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNameIAU source namemeta.id;meta.mainIndex1index of shining rate (1)stat.paramVx1/ccomponent of expansion velocity in the observer direction (1)phys.veloc.expansionINC1flux incorrectness (for the best fit case) (1)%stat.errorinc1shape incorrectness (for the best fit case)(1)%stat.errorIndex2[]? index of shining rate (2)stat.paramVx2/c[]? component of the expansion velocity in the observer direction (2)phys.veloc.expansionINC2[]? flux incorrectness (for the best fit case)(2)%stat.errorinc2[]? shape incorrectness (for the best fit case)(2)%stat.errorIndex3index of shining rate (3)stat.paramB3difference in twins positions (3)%stat.fit.paramINC3flux incorrectness (for the best fit case)(3)%stat.errorinc3[]? shape incorrectness (for the best fit case)(3)%stat.errorIndex4[]? index of shining rate (4)stat.paramB4[]? difference in twins positions (4)%stat.fit.paramINC4[]? flux incorrectness (for the best fit case)(4)%stat.errorinc4[]? shape incorrectness (for the best fit case)(4)%stat.error
ivo://CDS.VizieR/J/A+A/281/3552019-06-21T18:30:00ZJ.A_Aivo_managed1X-ray AGN content of Molonglo 408MHz survey (Brinkmann+ 1994)J/A+A/281/355ivo://CDS.VizieR/J/A+A/281/355CDSBRINKMANN W., SIEBERT J., BOLLER T.Patricia Bauer [CDS]1997-12-09T17:15:4713-Oct-1993CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frAGNThe cross-correlation of a source list from the ROSAT All-Sky Survey with the Molonglo 408MHz survey (MRC) yields to a catalogue of 549 sources. The majority of the objects are quasars and radio galaxies with known optical counterparts; more than one third of the objects are optically unidentified. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/281/355CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/281/355http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/281/355GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapX-rayRadio
J/A+A/281/355/table2MRC-ROSAT sources with identificationsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordMRCMRC identificationmeta.id;meta.mainF(408)408 MHz fluxJyphot.flux.density;em.radio.200-400MHzMorph[ AECMN] Morphology flag (1)src.morph.typeRef[ PSMCRT] Cross-reference flag (2)meta.refTypeType of optical counterpart with some further specifications about its naturesrc.classMv[]? Optical magnitudemagphot.mag;em.opt.Vl_Zlimit flag on redshiftmeta.code.errorZ[]? Redshiftsrc.redshiftNameCommon name of the sourcemeta.idRosatRosat designationmeta.idDOffset between X-ray and MRC radio positionarcsecpos.angDistanceFxX-ray fluxmW/m2phot.flux;em.X-raye_FxError for the X-ray fluxmW/m2stat.error
ivo://CDS.VizieR/J/A+A/281/8172019-06-21T18:30:00ZJ.A_Aivo_managed1Model atmospheres for Vega (Castelli+ 1994)J/A+A/281/817ivo://CDS.VizieR/J/A+A/281/817CDSCASTELLI F., KURUCZ R.L.Patricia Bauer [CDS]1997-12-09T17:16:3812-Nov-1993CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frStarsModels(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/281/817CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/281/817http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/281/817GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tap
J/A+A/281/817/table4aThe 9550K, log g = 3.98 ATLAS12 model for Vega abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordRhoxMass depth variable = integral(0 to x)(rho(x)dx)g/cm2phys.columnDensityTTemperatureKphys.temperaturePGas pressure0.1Paphys.pressureNeElectron number densitycm-3phys.densityAbRossRosseland mass absorption coefficientcm2/gphys.absorption.coeffAccRadRadiative accelerationcm/s2phys.accelerationVturbMicroturbulence velocitycm/sphys.veloc.microTurb
J/A+A/281/817/table2bAbundance change for table2arecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNelemAtomic number of the elementphys.atmol.numberACAbundance change (log(Nelem/Ntot)phys.abund
J/A+A/281/817/table5bAbundance change for table5arecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNelemAtomic number of the elementphys.atmol.numberACAbundance change (log(Nelem/Ntot)phys.abund
J/A+A/281/817/table4bAbundance change for table4arecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNelemAtomic number of the elementphys.atmol.numberACAbundance change (log(Nelem/Ntot)phys.abund
J/A+A/281/817/table3aThe 9550K, log g = 3.95 ATLAS12 model for Vega abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordRhoxMass depth variable = integral(0 to x)(rho(x)dx)g/cm2phys.columnDensityTTemperatureKphys.temperaturePGas pressure0.1Paphys.pressureNeElectron number densitycm-3phys.densityAbRossRosseland mass absorption coefficientcm2/gphys.absorption.coeffAccRadRadiative accelerationcm/s2phys.accelerationVturbMicroturbulence velocitycm/sphys.veloc.microTurb
J/A+A/281/817/table5aThe 9600K, log g = 4.00 ATLAS12 model for Vega abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordRhoxMass depth variable = integral(0 to x)(rho(x)dx)g/cm2phys.columnDensityTTemperatureKphys.temperaturePGas pressure0.1Paphys.pressureNeElectron number densitycm-3phys.densityAbRossRosseland mass absorption coefficientcm2/gphys.absorption.coeffAccRadRadiative accelerationcm/s2phys.accelerationVturbMicroturbulence velocitycm/sphys.veloc.microTurb
J/A+A/281/817/table2aThe 9600K, log g = 4.00, [M/H] = -0.5 ATLAS9 model for N(He)/Ntot = 0.0634recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordRhoxMass depth variable = integral(0 to x)(rho(x)dx)g/cm2phys.columnDensityTTemperatureKphys.temperaturePGas pressure0.1Paphys.pressureNeElectron number densitycm-3phys.densityAbRossRosseland mass absorption coefficientcm2/gphys.absorption.coeffAccRadRadiative accelerationcm/s2phys.accelerationVturbMicroturbulence velocitycm/sphys.veloc.microTurb
J/A+A/281/817/table1aThe 9550K, log g = 3.95, [M/H] = -0.5 ATLAS9 model for solar He abundancerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordRhoxMass depth variable = integral(0 to x)(rho(x)dx)g/cm2phys.columnDensityTTemperatureKphys.temperaturePGas pressure0.1Paphys.pressureNeElectron number densitycm-3phys.densityAbRossRosseland mass absorption coefficientcm2/gphys.absorption.coeffAccRadRadiative accelerationcm/s2phys.accelerationVturbMicroturbulence velocitycm/sphys.veloc.microTurb
J/A+A/281/817/table1bAbundance change for table1arecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNelemAtomic number of the elementphys.atmol.numberACAbundance change (log(Nelem/Ntot)phys.abund
J/A+A/281/817/table3bAbundance change for table3arecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNelemAtomic number of the elementphys.atmol.numberACAbundance change (log(Nelem/Ntot)phys.abund
ivo://CDS.VizieR/J/A+A/282/L92019-06-21T18:30:00ZJ.A_Aivo_managed1"flip-flop" in FK Com (Jetsu+ 1994)J/A+A/282/L9ivo://CDS.VizieR/J/A+A/282/L9CDSJETSU L., TUOMINEN I., GRANKIN K.N., MEL'NIKOV S.YU., SHEVCHENKO V.S.Francois Ochsenbein [CDS]1997-12-09T17:17:1711-Feb-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometry:wide-bandStars:variable(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/282/L9CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/282/L9http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/282/L9GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOpticalInfrared
J/A+A/282/L9/table1Two new subsets of UBVR (standard Johnson) photometry of FK Com.recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordSET[59/60] Subset numbermeta.idHJD[2448415/2448864]+ Heliocentric Julian daydtime.epochU[9/9.9]? U magnitudemagphot.mag;em.opt.UBB magnitudemagphot.mag;em.opt.BVV magnitudemagphot.mag;em.opt.VR[7/8]? R magnitudemagphot.mag;em.opt.RF[0/2] Flare detection : F=0: normal flare F=1: flare (detected with U-band) F=2: flare? (detected without U-band)meta.code
ivo://CDS.VizieR/J/A+A/283/9112019-06-21T18:30:00ZJ.A_Aivo_managed1Abundances in NGC 2243 and Mel 66 (Gratton+ 1994)J/A+A/283/911ivo://CDS.VizieR/J/A+A/283/911CDSGRATTON R.G., CONTARINI G.Patricia Bauer [CDS]1997-12-09T17:17:5022-Oct-1993CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frAbundancesOpen_ClustersSpectroscopy(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/283/911CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/283/911http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/283/911GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/283/911/table1Equivalent widths and abundances of lines in the spectra of giants in NGC 2243 and Mel 66recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordSpecieSpeciephys.atmol.elementLambdaLine wavelength0.1nmem.wlEPExcitation energyeVphys.energy;phys.atmol.excitationlog(gf)Oscillator strengthphys.atmol.wOscStrengthn[ *] A * marks lines with detailed HFS analysismeta.noteEW4110[]? Equivalent width for star 4110 in NGC22430.1pmspect.line.eqWidthn_EW4110[ s] When s, the line was saturatedmeta.notelog(A4110)[]? Abundance for star 4110 in NGC2243 (1)phys.abundEW4209[]? Equivalent width for star 4209 in NGC22430.1pmspect.line.eqWidthn_EW4209[ s] When s, the line was saturatedmeta.notelog(A4209)[]? Abundance for star 4209 in NGC2243 (1)phys.abundEW1242[]? Equivalent width for star 1242 in Mel 660.1pmspect.line.eqWidthn_EW1242[ s] When s, the line was saturatedmeta.notelog(A1242)[]? Abundance for star 1242 in Mel 66 (1)phys.abundEW4151[]? Equivalent width for star 4151 in Mel 660.1pmspect.line.eqWidthn_EW4151[ s] When s, the line was saturatedmeta.notelog(A4154)[]? Abundance for star 4154 in Mel 66 (1)phys.abund
ivo://CDS.VizieR/J/A+A/284/5152019-06-21T18:30:00ZJ.A_Aivo_managed1Long-term periodic variability in gamma Cas (Telting+ 1994)J/A+A/284/515ivo://CDS.VizieR/J/A+A/284/515CDSTELTING J.H., KAPER L.Patricia Bauer [CDS]1997-12-09T17:18:1718-Jan-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frSpectroscopyStars:EmissionStars:variable(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/284/515CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/284/515http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/284/515GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/284/515/table4Results of fitting the model to residual spectra of gamma CasrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNameImage numbermeta.id;meta.mainVc1N V best-fitting of the Vc Discret Absorption Component (DAC) model parameterkm/sphys.veloc;pos.heliocentrice_Vc1rms uncertainty on Vc for N Vkm/sstat.errorTau_c1N V best-fitting of the Tau_c DAC parameterstat.parame_Tau_c1rms uncertainty on Tau_c for N Vstat.errorVt1N V best-fitting of the Vt DAC parameterkm/sphys.veloc;pos.heliocentrice_Vt1rms uncertainty on Vt for N Vkm/sstat.errorNcol1N V column density10+12cm-2phys.columnDensitye_Ncol1rms uncertainty on Ncol for N V10+12cm-2stat.errorKhi21[]? N V reduced Khi2 value of the best fitstat.fit.paramVc2Si IV best-fitting of the Vc DACparameterkm/sstat.fit.parame_Vc2rms uncertainty on Vc for Si IVkm/sstat.errorTau_c2Si IV best-fitting of the Tau_c DAC parameterstat.parame_Tau_c2rms uncertainty on Tau_c for Si IVstat.errorVt2Si IV best-fitting of the Vt DAC parameterkm/sphys.veloc;pos.heliocentrice_Vt2rms uncertainty on Vt for Si IVkm/sstat.errorNcol2Si IV column density10+12cm-2phys.columnDensitye_Ncol2rms uncertainty on Ncol for Si IV10+12cm-2stat.errorKhi22[]? Si IV reduced Khi2 value of the best fitstat.fit.paramVc3C IV best-fitting of the Vc DAC parameterkm/sstat.fit.parame_Vc3rms uncertainty on Vc for C IVkm/sstat.errorTau_c3C IV best-fitting of the Tau_c DAC parameterstat.parame_Tau_c3rms uncertainty on Tau_c for C IVstat.errorVt3C IV best-fitting of the Vt DAC parameterkm/sphys.veloc;pos.heliocentrice_Vt3rms uncertainty on Vt for C IVkm/sstat.errorNcol3C IV column density10+12cm-2phys.columnDensitye_Ncol3rms uncertainty on Ncol for C IV10+12cm-2stat.errorKhi23[]? C IV reduced Khi2 value of the best fitstat.fit.param
ivo://CDS.VizieR/J/A+A/285/12019-06-21T18:30:00ZJ.A_Aivo_managed1Spectrographic study of Kiso UV-excess galaxies (Comte+ 1994)J/A+A/285/1ivo://CDS.VizieR/J/A+A/285/1CDSCOMTE G., AUGARDE R., CHALABAEV A., KUNTH D., MAEHARA H.Patricia Bauer [CDS]1997-12-09T17:18:3319-Oct-1993CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frGalaxiesSpectroscopy(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/285/1CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/285/1http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/285/1GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapUV
J/A+A/285/1/table6Relative line ratios and oxygen abundances for 92 KUGsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordKUGGalaxy KUG number (in Kiso Catalog)meta.id;meta.main[OII]log ([OII]/Hbeta)spect.line.intensity;arith.ratio[OIII][]? log ([OIII]/Hbeta)spect.line.intensity;arith.ratio[OI][]? log ([OI]/Hbeta)spect.line.intensity;arith.ratio[NII][]? log ([NII]/Hbeta)spect.line.intensity;arith.ratio[SII][]? log ([SII]/Hbeta)spect.line.intensity;arith.ratioE(B-V)E(B-V) from Balmer decrementphot.color.excessTe[]? Electron temperature of the HII zoneKphys.temperature;phys.electron12+log(O/H)[]? 12 + log([O/H]) (oxygen abundance)phys.abund
ivo://CDS.VizieR/J/A+A/285/4592019-06-21T18:30:00ZJ.A_Aivo_managed1RZ Dra (Kreiner+ 1994)J/A+A/285/459ivo://CDS.VizieR/J/A+A/285/459CDSKREINER J.M., PAJDOSZ G., TREMKO J., ZOLA S.Patricia Bauer [CDS]1997-12-09T17:19:0527-Jan-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frBinaries:eclipsingPhotometry:wide-band(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/285/459CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/285/459http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/285/459GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/285/459/table2Differential V photometry of RZ DrarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNNumber of observationsmeta.numberHDJHeliocentric Julian Datedtime.epochdVmagDifferential V magnitude (variable-comparison)magphot.mag;arith.diff
J/A+A/285/459/table1Differential B photometry of RZ DrarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNNumber of observationsmeta.numberHJDHeliocentric Julian Datedtime.epochdBmagDifferential B magnitude (variable-comparison)magphot.mag;arith.diff
ivo://CDS.VizieR/J/A+A/285/8122019-06-21T18:30:00ZJ.A_Aivo_managed1Spectral properties of X-ray extragal. sources (Brinkmann+ 1994)J/A+A/285/812ivo://CDS.VizieR/J/A+A/285/812CDSBRINKMANN W., SIEBERT J.Patricia Bauer [CDS]1997-12-09T17:19:4223-Feb-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frGalaxies(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/285/812CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/285/812http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/285/812GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapX-rayUVRadio
J/A+A/285/812/table1Spectral properties of X-ray loud extragalactic radio sourcesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordROSATROSAT name (position J2000.0)meta.id;meta.mainNameOther name of the sourcemeta.idTypeOptical identification given in the NEDmeta.idGammaX-ray spectral indexspect.indexe_Gammarms uncertainty on X-ray spectral indexstat.errorN(H)Absorbing neutral hydrogen column density (best fit)10+21cm-2phys.columnDensitye_N(H)rms uncertainty on N(H)10+21cm-2stat.errorchi2Reduced chi2 for the fit (Errors are 1 sigma)stat.fit.paramnu[]? Degrees of freedom for chi2stat.fit.dofGammaN(H)gX-ray spectral index for fixed galactic N(H)spect.indexe_GammaN(H)grms uncertainty on GammaN(H)gstat.errorN(H)gAbsorbing neutral hydrogen column density for fixed galactic N(H)10+21cm-2phys.columnDensitychi2(g)Reduced chi2 for the fit for fixed galactic N(H) (Errors are 1 sigma)stat.fit.paramnu(g)[]? Degrees of freedom for chi2(g)stat.fit.paramfXUnabsorbed X-ray flux in the total ROSAT energy band, computed by using the best fit values for Gamma and N(H)10-11mW/m2phot.flux;em.X-rayfradRadio flux at 5 GHz (Green Bank sources) or 408 MHz (Molonglo sources)Jyphot.flux.density;em.radio.3-6GHzn_fradnote (1)meta.noterefReferencesmeta.ref
ivo://CDS.VizieR/J/A+A/286/1362019-06-21T18:30:00ZJ.A_Aivo_managed1Radial velocities of four beta Cep variables (Aerts+ 1994)J/A+A/286/136ivo://CDS.VizieR/J/A+A/286/136CDSAERTS C., WAELKENS C., DE PAUW M.Patricia Bauer [CDS]1997-12-09T17:19:5931-Jan-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frVelocitiesStars:variable(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/286/136CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/286/136http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/286/136GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/286/136/table12HJD and radial velocities for the measured spectra of the four stars (table12 + table13 in the paper)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHJD1[]? Heliocentric Julian Date for KK Vel (1)dtime.epoch<v>1[]? Radial velocity for KK Velkm/sphys.veloc;pos.heliocentricHJD2[]? Heliocentric Julian Date for nu Eri (1)dtime.epoch<v>2[]? Radial velocity for nu Erikm/sphys.veloc;pos.heliocentricHJD3[]? Heliocentric Julian Date for beta CMa (1)dtime.epoch<v>3[]? Radial velocity for beta CMakm/sphys.veloc;pos.heliocentricHJD4Heliocentric Julian Date for V348 Nor (1)dtime.epoch<v>4Radial velocity FOR V348 Norkm/sphys.veloc;pos.heliocentric
ivo://CDS.VizieR/J/A+A/286/4442019-06-21T18:30:00ZJ.A_Aivo_managed1The globular cluster NGC 6652 (Ortolani+ 1994)J/A+A/286/444ivo://CDS.VizieR/J/A+A/286/444CDSORTOLANI S., BICA E., BARBUY B.Patricia Bauer [CDS]1997-12-09T17:20:4117-Nov-1993CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frGlobular_ClustersStarsPhotometry:wide-band(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/286/444CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/286/444http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/286/444GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOpticalInfrared
J/A+A/286/444/table3V, I photometry in NGC 6652recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordSeqSequence numbermeta.id;meta.mainXposX pixel coordinate as in Fig. 1pos.cartesian.x;instr.detYposY pixel coordinate as in Fig. 1pos.cartesian.y;instr.detVmagV magnitudemagphot.mag;em.opt.VV-IV-I colourmagphot.color;em.opt.V;em.opt.I
J/A+A/286/444/table2B, V photometry in NGC 6652recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordSeqSequence numbermeta.id;meta.mainXposX pixel coordinate as in Fig. 1pos.cartesian.x;instr.detYposY pixel coordinate as in Fig. 1pos.cartesian.y;instr.detVmagV magnitudemagphot.mag;em.opt.VB-VB-V colourmagphot.color;em.opt.B;em.opt.V
ivo://CDS.VizieR/J/A+A/287/5912019-06-21T18:30:00ZJ.A_Aivo_managed1UV Variations in spectrum of Abell 35 c.star (Jasniewicz+ 1994)J/A+A/287/591ivo://CDS.VizieR/J/A+A/287/591CDSJASNIEWICZ G., LAPIERRE G., MONIER R.Patricia Bauer [CDS]1997-12-09T17:20:5917-Mar-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometry:wide-bandStars:variable(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/287/591CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/287/591http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/287/591GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/287/591/table2Photometric observations of BD-22 3467 carried out in 1992 in the Geneva photometric systemrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordJDJulian daydtime.epochVmagVisual magnitudemagphot.mag;em.opt.VU-BU-B colormagphot.color;em.opt.U;em.opt.BB-VB-V colormagphot.color;em.opt.B;em.opt.V
ivo://CDS.VizieR/J/A+A/287/8172019-06-21T18:30:00ZJ.A_Aivo_managed1Period changes in RT Lac (Keskin+ 1994)J/A+A/287/817ivo://CDS.VizieR/J/A+A/287/817CDSKESKIN V., IBANOGLU M.C., AKAN C., EVREN S., TUNCA Z.Patricia Bauer [CDS]1997-12-09T17:21:1825-Feb-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frBinaries:eclipsingStars:variable(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/287/817CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/287/817http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/287/817GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/287/817/table2Up-dated times of primary and secondary eclipses and residualsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordMinTime of minima in Julian daydtime.epochEInteger eclipse cycle numbermeta.number;time.periodO-C(I)Observed-calculated residual for primary minimadstat.fit.omc;timeO-C(II)[]? Observed-calculated residual for secondary minimadstat.fit.omc;timeRefReferences: (1) Hall & Kreiner (1980) (2) Ibanoglu et al. (1980) (3) Tunca et al. (1983) (4) Evren (1989) (5) This papermeta.note
ivo://CDS.VizieR/J/A+A/287/9272019-06-21T18:30:00ZJ.A_Aivo_managed1Abundances for lines of n-capture in 19 stars (Gratton+ 1994)J/A+A/287/927ivo://CDS.VizieR/J/A+A/287/927CDSGRATTON R.G., SNEDEN C.Patricia Bauer [CDS]1997-12-09T17:21:3631-Jan-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frAbundancesStarsSpectroscopy(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/287/927CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/287/927http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/287/927GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/287/927/table3Equivalent widths and abundances for lines of n-capture elements in 19 metal-poor starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHDHD namemeta.id;meta.mainEElementphys.atmol.elementWWavelength0.1nmem.wlEPPotential energyeVphys.energy;phys.atmol.levellog(gf)Oscillator strengthphys.atmol.wOscStrengthl_EWLimit flag on equivalent widthmeta.code.errorEW[]? Equivalent width0.1pmspect.line.eqWidthn[ s] When s, the line was saturatedmeta.notel_log(A)Limit flag on abundancemeta.code.errorlog(A)[]? Abundancephys.abund
ivo://CDS.VizieR/J/A+A/288/4132019-06-21T18:30:00ZJ.A_Aivo_managed1Massive stars in I Zw 36 (Deharveng+ 1994)J/A+A/288/413ivo://CDS.VizieR/J/A+A/288/413CDSDeharveng J.-M., Albrecht R., Barbieri C., Blades J.C., Boksenberg A., Crane P., Disney M.J., Jakobsen P., Kamperman T.M., King I.R., Macchetto F., Mackay C.D., Paresce F., Weigelt G., Baxter D., Greenfield P., Jedrzejewski R., Nota A., Sparks W.B.James Marcout, Patricia Bauer [CDS]1997-12-09T17:21:5228-Jan-1997CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometryWe have observed the blue dwarf galaxy I Zw 36 with the f/96 relay of the HST Faint Object Camera and have for the first time resolved massive stars, using the broad band filters F175W, F342W, F430W and F480LP. We have measured the fluxes of 143 of these objects and studied their characteristics in color-magnitude diagrams. A few stars may be red supergiants but their contribution to the integrated light is less than 5% in the F430W filter. The F175W-F430W color of the integrated stellar population is redder than expected from the current burst of star formation, suggesting therefore the presence of an older and unresolved underlying population. The ultraviolet measurements combined with synthetic photometry calculations allow us to place the massive stars in a bolometric magnitude vs. temperature diagram. In this diagram, the stars are compared to evolutionary tracks for different stellar masses. The current burst probably has an age less than 12Myr. We infer an Initial Mass Function, with a power-law slope in the range -1.7 to -2.6 for masses M>=20M_{sun}_. This is consistent with most of the values reported for sites of star formation in the Galaxy and the Magellanic Clouds and does not support the view of an IMF flattening at low metallicity. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/288/413CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/288/413http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/288/413GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapHSTUV
J/A+A/288/413/table1Photometry of starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIDIdentification numbermeta.id;meta.mainXposX position (1)pixpos.cartesian.x;instr.detYposY position (1)pixpos.cartesian.y;instr.detm175? Magnitude through the F175W filtermagphot.mag;em.UV.100-200nmm342? Magnitude through the F342W filtermagphot.mag;em.opt.Um430Magnitude through the F430W filtermagphot.mag;em.opt.B
ivo://CDS.VizieR/J/A+A/288/6012019-06-21T18:30:00ZJ.A_Aivo_managed1Dense molecular cores (Zinchenko+ 1994)J/A+A/288/601ivo://CDS.VizieR/J/A+A/288/601CDSZINCHENKO I., FORSSTROEM V., LAPINOV A., MATTILA K.Patricia Bauer [CDS]1997-12-09T17:22:0923-Mar-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frInterstellar_MediumSpectroscopy(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/288/601CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/288/601http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/288/601GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/288/601/table6CS mapping data for S184recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordDalphaGaussian line parameter Delta(alpha)arcminspect.line.widthDdeltaGaussian line parameter, Delta(delta)arcminspect.line.widthl_TR*limit flag on TR*meta.code.errorTR*Temperature scale (1)Kphys.temperaturee_TR*[]? rms uncertainty on TR*Kstat.errorDeltaV[]? Line broadeningkm/sspect.line.broade_DeltaV[]? rms uncertainty on DeltaVkm/sstat.errorVlsr[]? LSR velocitykm/sphys.veloc;pos.lsre_Vlsr[]? rms uncertainty on Vlsrkm/sstat.error
J/A+A/288/601/table7CS mapping data for S199recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordDalphaGaussian line parameter Delta(alpha)arcminspect.line.widthDdeltaGaussian line parameter, Delta(delta)arcminspect.line.widthl_TR*limit flag on TR*meta.code.errorTR*Temperature scale (1)Kphys.temperaturee_TR*[]? rms uncertainty on TR*Kstat.errorDeltaV[]? Line broadeningkm/sspect.line.broade_DeltaV[]? rms uncertainty on DeltaVkm/sstat.errorVlsr[]? LSR velocitykm/sphys.veloc;pos.lsre_Vlsr[]? rms uncertainty on Vlsrkm/sstat.error
J/A+A/288/601/table8CS mapping data for S255recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordDalphaGaussian line parameter Delta(alpha)arcminspect.line.widthDdeltaGaussian line parameter, Delta(delta)arcminspect.line.widthl_TR*limit flag on TR*meta.code.errorTR*Temperature scale (1)Kphys.temperaturee_TR*[]? rms uncertainty on TR*Kstat.errorDeltaV[]? Line broadeningkm/sspect.line.broade_DeltaV[]? rms uncertainty on DeltaVkm/sstat.errorVlsr[]? LSR velocitykm/sphys.veloc;pos.lsre_Vlsr[]? rms uncertainty on Vlsrkm/sstat.error
J/A+A/288/601/table5CS mapping data for S159recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordDalphaGaussian line parameter Delta(alpha)arcminspect.line.widthDdeltaGaussian line parameter, Delta(delta)arcminspect.line.widthl_TR*limit flag on TR*meta.code.errorTR*Temperature scale (1)Kphys.temperaturee_TR*[]? rms uncertainty on TR*Kstat.errorDeltaV[]? Line broadeningkm/sspect.line.broade_DeltaV[]? rms uncertainty on DeltaVkm/sstat.errorVlsr[]? LSR velocitykm/sphys.veloc;pos.lsre_Vlsr[]? rms uncertainty on Vlsrkm/sstat.error
J/A+A/288/601/table3CS mapping data for S76recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordDalphaGaussian line parameter Delta(alpha)arcminspect.line.widthDdeltaGaussian line parameter, Delta(delta)arcminspect.line.widthl_TR*limit flag on TR*meta.code.errorTR*Temperature scale (1)Kphys.temperaturee_TR*[]? rms uncertainty on TR*Kstat.errorDeltaV[]? Line broadeningkm/sspect.line.broade_DeltaV[]? rms uncertainty on DeltaVkm/sstat.errorVlsr[]? LSR velocitykm/sphys.veloc;pos.lsre_Vlsr[]? rms uncertainty on Vlsrkm/sstat.error
J/A+A/288/601/table4CS mapping data for S153recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordDalphaGaussian line parameter Delta(alpha)arcminspect.line.widthDdeltaGaussian line parameter, Delta(delta)arcminspect.line.widthl_TR*limit flag on TR*meta.code.errorTR*Temperature scale (1)Kphys.temperaturee_TR*[]? rms uncertainty on TR*Kstat.errorDeltaV[]? Line broadeningkm/sspect.line.broade_DeltaV[]? rms uncertainty on DeltaVkm/sstat.errorVlsr[]? LSR velocitykm/sphys.veloc;pos.lsre_Vlsr[]? rms uncertainty on Vlsrkm/sstat.error
ivo://CDS.VizieR/J/A+A/289/1372019-06-21T18:30:00ZJ.A_Aivo_managed1DK Cygni light curve (Awadalla, 1994)J/A+A/289/137ivo://CDS.VizieR/J/A+A/289/137CDSAWADALLA N.S.Patricia Bauer [CDS]1997-12-09T17:22:5118-Feb-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frBinaries:eclipsingPhotometry:wide-band(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/289/137CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/289/137http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/289/137GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/289/137/tableUBV photoelectric light curverecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHJDHeliocentric Julian daydtime.epochDeltaV[]? V differential magnitudemagphot.mag;arith.diffDeltaB[]? B differential magnitudemagphot.mag;arith.diffDeltaU[]? U differential magnitudemagphot.mag;arith.diff
ivo://CDS.VizieR/J/A+A/289/7402019-06-21T18:30:00ZJ.A_Aivo_managed1Galactic abundance gradients (Kaufer+, 1994)J/A+A/289/740ivo://CDS.VizieR/J/A+A/289/740CDSKAUFER A., SZEIFERT T., KRENZIN R., BASCHEK B., WOLF B.Patricia Bauer [CDS]1997-12-09T17:23:0403-May-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frAbundancesSpectroscopyStars:early-type(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/289/740CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/289/740http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/289/740GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/289/740/table7Measured equivalent widthrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIdent.Laboratory wavelengths of the contributing line componentsmeta.id;spect.lineHR1763[]? Measured equivalent width for HR1763pmspect.line.eqWidthHR1765[]? Measured equivalent width for HR1765pmspect.line.eqWidthHR1842[]? Measured equivalent width for HR1842pmspect.line.eqWidthHR1886[]? Measured equivalent width for HR1886pmspect.line.eqWidthHR1887[]? Measured equivalent width for HR1887pmspect.line.eqWidth
J/A+A/289/740/table6Measured equivalent widthrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIdent.Laboratory wavelengths of the contributing line componentsmeta.id;spect.lineNGC6531/2[]? Measured equivalent width for NGC6531/2pmspect.line.eqWidthNGC6823/34[]? Measured equivalent width for NGC6823/34pmspect.line.eqWidthNGC6910/2[]? Measured equivalent width for NGC6910/2pmspect.line.eqWidthNGC1893/9[]? Measured equivalent width for NGC1893/9pmspect.line.eqWidthNGC1893/10[]? Measured equivalent width for NGC1893/10pmspect.line.eqWidth
J/A+A/289/740/table2List of the starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNameObject namemeta.id;meta.mainRef.Reference (1)meta.refVvisual magnitudemagphot.mag;em.opt.VDgalgalactocentric distancekpcpos.distance
J/A+A/289/740/table8Measured equivalent widthrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIdent.Laboratory wavelengths of the contributing line componentsmeta.id;spect.linehPer/717[]? Measured equivalent width for hPer/717pmspect.line.eqWidthhPer/782[]? Measured equivalent width for hPer/782pmspect.line.eqWidthS247/1[]? Measured equivalent width for S247/1pmspect.line.eqWidthS301/3[]? Measured equivalent width for S301/3pmspect.line.eqWidthS217/3[]? Measured equivalent width for S217/3pmspect.line.eqWidthS208/6[]? Measured equivalent width for S208/6pmspect.line.eqWidth
ivo://CDS.VizieR/J/A+A/289/8712019-06-21T18:30:00ZJ.A_Aivo_managed1YY Eri & AE Phe (Maceroni+, 1994)J/A+A/289/871ivo://CDS.VizieR/J/A+A/289/871CDSMACERONI C., VAN'T VEER F.Patricia Bauer [CDS]1997-12-09T17:23:1606-May-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frBinaries:spectroscopicPhotometry:wide-band(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/289/871CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/289/871http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/289/871GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/289/871/yyeriJohnson BV observations of YY ErirecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHJDHeliocentric Julian daydtime.epochU[]? U differential magnitude (variable-comparison)magphot.mag;arith.diffB[]? B differential magnitude (variable-comparison)magphot.mag;arith.diffV[]? V differential magnitude (variable-comparison)magphot.mag;arith.diff
J/A+A/289/871/aepheJohnson UBV observations of AE PherecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHJDHeliocentric Julian daydtime.epochU[]? U differential magnitude (variable-comparison)magphot.mag;arith.diffB[]? B differential magnitude (variable-comparison)magphot.mag;arith.diffV[]? V differential magnitude (variable-comparison)magphot.mag;arith.diff
ivo://CDS.VizieR/J/A+A/290/6092019-06-21T18:30:00ZJ.A_Aivo_managed1Be stars near-IR excess (Dougherty+, 1994)J/A+A/290/609ivo://CDS.VizieR/J/A+A/290/609CDSDOUGHERTY S.M., WATERS L.B.F.M., BURKI G., COTE J., CRAMER N., VAN KERKWIJK M.H., TAYLOR A.R.Patricia Bauer [CDS]1997-12-09T17:23:2830-May-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frStars:early-type(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/290/609CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/290/609http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/290/609GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/290/609/table1Excess colours of 144 Be starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHR[]? HR numbermeta.idHDHD numbermeta.id;meta.mainSourceSource namemeta.idSpSpectral type (from the Bright Star Catalogue)src.spTypeE[B-V]1Excess [B-V] colour (calculated from spectral type)magphot.color.excessE[B-V]2[]? Excess [B-V] colour from the 2175 angstrom interstellar absorption feature (Beeckmans and Hubert-Delplace (1980)) and converted using E(B-V) = 0.84E[B-V] (Cramer, 1984)magphot.color.excessE[V-J]Excess [V-J] colourmagphot.color.excessE[V-H][]? Excess [V-H] colourmagphot.color.excessE[V-K][]? Excess [V-K] colourmagphot.color.excessE[V-L][]? excess [V-L] colourmagphot.color.excessRefComment for the source of the observations: a) Dougherty et al., 1991 b) Dachs et al., 1988 c) Burki et al., in preparation Visual observations from Burki et al. (in preparation) except when n_Ref. = 5meta.noten_RefIf n_Ref = 5, the visual observations are taken from the catalogue of Rufener (1988)meta.note
ivo://CDS.VizieR/J/A+A/290/692019-06-21T18:30:00ZJ.A_Aivo_managed1M3 photographic photometry (Buonanno+, 1994)J/A+A/290/69ivo://CDS.VizieR/J/A+A/290/69CDSBUONANNO R., CORSI C.E., BUZZONI A., CACCIARI C., FERRARO F.R., FUSI PECCI F.Patricia Bauer [CDS]1997-12-09T17:23:4707-Nov-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frGlobular_ClustersPhotometry:wide-bandA new photographic colour-magnitude diagram for the Galactic globular cluster M 3 is presented. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/290/69CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/290/69http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/290/69GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/290/69/table6Remaining 9491 starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNameIdentification numbermeta.id;meta.mainm_NameMultiplicity index on Namemeta.code.multipVmagV magnitudemagphot.mag;em.opt.VBmagB magnitudemagphot.mag;em.opt.BB-VB-V colourmagphot.color;em.opt.B;em.opt.VXX positionarcsecpos.cartesianYY positionarcsecpos.cartesian
J/A+A/290/69/table4Complete Bright Total sample (excluding the 96 known variables)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNameIdentification numbermeta.id;meta.mainm_NameMultiplicity index on Namemeta.code.multipVmagV magnitudemagphot.mag;em.opt.VBmagB magnitudemagphot.mag;em.opt.BB-VB-V colourmagphot.color;em.opt.B;em.opt.VXX positionarcsecpos.cartesianYY positionarcsecpos.cartesian
ivo://CDS.VizieR/J/A+A/291/1102019-06-21T18:30:00ZJ.A_Aivo_managed1ER Vulpeculae (Olah+, 1994)J/A+A/291/110ivo://CDS.VizieR/J/A+A/291/110CDSOLAH K., BUDDING E., KIM H.-I., ETZEL P.B.Patricia Bauer [CDS]1997-12-09T17:24:1330-Jun-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frBinaries:eclipsingPhotometry:wide-band(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/291/110CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/291/110http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/291/110GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOpticalInfrared
J/A+A/291/110/tableUBV(RI)c photometry of ER VulrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordJDHHeliocentric Julian daydtime.epochU[]? U magnitudemagphot.mag;em.opt.UB[]? B magnitudemagphot.mag;em.opt.BV[]? V magnitudemagphot.mag;em.opt.VRc[]? Rc magnitudemagphot.mag;em.opt.RIc[]? Ic magnitudemagphot.mag;em.opt.I
ivo://CDS.VizieR/J/A+A/291/1212019-06-21T18:30:00ZJ.A_Aivo_managed1Study of star V9 in 47 Tuc (Storm+ 1994)J/A+A/291/121ivo://CDS.VizieR/J/A+A/291/121CDSSTORM J., NORDSTROEM B., CARNEY B.W., ANDERSEN J.Patricia Bauer [CDS]1997-12-09T17:24:2812-Apr-1996CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frVelocitiesStars:variableWe present an infrared K-band light curve and a radial velocity curve for the RR Lyrae star V9 in the metal rich globular cluster 47 Tucanae ([Fe/H]=-0.71). Combining these new data with the optical photometry presented in Carney et al. (1993PASP..105..294C), we perform a Baade-Wesselink analysis and derive a distance modulus of 47 Tuc of 13.23mag+/-0.17 and absolute mean magnitudes of <M_V_>=0.32mag and <M_K_>=-0.57mag for V9. We also present a well populated visual-infrared color-magnitude diagram of the cluster, reaching from the upper red giant branch to the subgiant branch. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/291/121CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/291/121http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/291/121GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapInfrared
J/A+A/291/121/table3Radial velocities for V9 in 47 TucrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHJDHeliocentric Julian Date at mid-exposuredtime.epochPhase[0/1[ Phase computed according to the ephemeris HJD(max) = 2447485.385 + 0.736852 * E (days)time.phaseRVRadial velocitykm/sphys.veloc;pos.heliocentrice_RVrms uncertainty on RVkm/sstat.errorDepth? Depth of the CORAVEL cross-correlation dipphot.flux.density;arith.ratioe_Depth? rms uncertainty on Depthstat.errorWidth? Width of the CORAVEL cross-correlation dipkm/sobs.parame_Width? rms uncertainty on Widthkm/sstat.errorNAverage number of counts per channel for the measurementphot.count;em.opt
J/A+A/291/121/table1K magnitudes for V9recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHJDHeliocentric Julian Date at mid-exposuredtime.epochPhase[0/1[ Phase computed according to the ephemeris HJD(max) = 2447485.385 + 0.736852 * E (days)time.phaseKmagAverage K-band magnitude computed after binning the data according to time in bins of 11 measurements and rejecting 3 sigma outliers iteratively.magphot.mag;em.IR.Ke_Kmagrms uncertainty on Kmagmagstat.error
J/A+A/291/121/table2Infrared-optical color-magnitude data for 47 TucrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIDSequential numbermeta.id;meta.mainXposX coordinate in the IR detector framepixpos.cartesian.x;instr.detYposY coordinate in the IR detector framepixpos.cartesian.y;instr.detK0magDereddened K magnitude of the starmagphot.mag;em.IR.Ke_K0magrms uncertainty on K0magmagstat.error(V-K)0Dereddened (V-K) color of the starmagphot.color;em.opt.V;em.IR.Ke_(V-K)0rms uncertainty on (V-K)0magstat.error
ivo://CDS.VizieR/J/A+A/293/3472019-06-21T18:30:00ZJ.A_Aivo_managed1LMC F supergiants (Hill+, 1995)J/A+A/293/347ivo://CDS.VizieR/J/A+A/293/347CDSHILL V., ANDRIEVSKY S., SPITE M.Patricia Bauer [CDS]1997-12-09T17:25:2126-Jul-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frAbundancesStarsSpectroscopy(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/293/347CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/293/347http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/293/347GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/293/347/appendixLines used in the analysis, with their equivalent width and individual abundance for each of the nine investigated LMC supergiants and for Canopus.recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordLambdaCentral wavelength of the line0.1nmem.wlEl.Name of the elementphys.atmol.elementEl.Ion.Degree of ionization of the element (1 for neutral and 2 for ionized species)phys.atmol.ionizationXi(ex)Excitation potential of the lineeVphys.energy;phys.atmol.excitationlog(gf)Line transition probability in log scalephys.atmol.wOscStrengthWG244[]? Equivalent width of the line for star G2440.1nmspect.line.eqWidthn_AG244[* ] Note on the abundance determination (1)meta.noteAG244[]? Abundance normalised to the Sun for G244Sunphys.abundWG258[]? Equivalent Width of the line for star G2580.1nmspect.line.eqWidthn_AG258[* ] Note on the abundance determination (1)meta.noteAG258[]? Abundance normalised to the Sun for G258Sunphys.abundWG274[]? Equivalent Width of the line for star G2740.1nmspect.line.eqWidthn_AG274[* ] Note on the abundance determination (1)meta.noteAG274[]? Abundance normalised to the Sun for G274Sunphys.abundWG319[]? Equivalent Width of the line for star G3190.1nmspect.line.eqWidthn_AG319[* ] Note on the abundance determination (1)meta.noteAG319[]? Abundance normalised to the Sun for G319Sunphys.abundWG396[]? Equivalent Width of the line for star G3960.1nmspect.line.eqWidthn_AG396[* ] Note on the abundance determination (1)meta.noteAG396[]? Abundance normalised to the Sun for G396Sunphys.abundWG406[]? Equivalent Width of the line for star G4060.1nmspect.line.eqWidthn_AG406[* ] Note on the abundance determination (1)meta.noteAG406[]? Abundance normalised to the Sun for G406Sunphys.abundWG439[]? Equivalent Width of the line for star G4390.1nmspect.line.eqWidthn_AG439[* ] Note on the abundance determination (1)meta.noteAG439[]? Abundance normalised to the Sun for G439Sunphys.abundWG501[]? Equivalent Width of the line for star G5010.1nmspect.line.eqWidthn_AG501[* ] Note on the abundance determination (1)meta.noteAG501[]? Abundance normalised to the Sun for G501Sunphys.abundWG538[]? Equivalent Width of the line for star G5380.1nmspect.line.eqWidthn_AG538[* ] Note on the abundance determination (1)meta.noteAG538[]? Abundance normalised to the Sun for G538Sunphys.abundWCan[]? Equivalent Width of the line for Canopus (taken from Luck & Lambert, 1985 and Desikachary & Hearnshaw, 1982)0.1nmspect.line.eqWidthn_ACan[*# ] Note on the abundance determination (1)meta.noteACan[]? Abundance normalised to the Sun for CanopusSunphys.abund
ivo://CDS.VizieR/J/A+A/293/7032019-06-21T18:30:00ZJ.A_Aivo_managed1Outflow in M82 halo (McKeith+, 1995)J/A+A/293/703ivo://CDS.VizieR/J/A+A/293/703CDSMcKEITH C.D., GREVE A., DOWNES D., PRADA F.Patricia Bauer [CDS]1997-12-09T17:25:3526-Jul-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frGalaxies:spectraInterstellar_MediumVelocities(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/293/703CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/293/703http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/293/703GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/293/703/table2Position-velocity data of the minor axis outflowrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordn_LineLine type, EL = emission line, SL = scattered linemeta.noteLineLine denominationmeta.id;spect.lined1Distance along minor axis in arc seconds positive values: North - West, negative values: South - Eastarcsecpos.angDistanced2Distance along minor axis in linear scale, (1" equals 15pc)kpcpos.distanceVelMeasured velocity-systemic velocity (systemic velocity=200km/s)km/sphys.veloc
J/A+A/293/703/table3Intensities of the blue to red velocity componentrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordLineLine denominationmeta.id;spect.lined1Distance along minor axis in arc seconds, positive values: North - West, negative values: South - Eastarcsecpos.angDistanced2Distance along minor axis in linear scale, (1" equals 15pc)kpcpos.distanceIBIntensity of blue shifted component (in relative linear units)spect.line.intensity;arith.ratioIRIntensity of red shifted component (in relative linear units)spect.line.intensity;arith.ratio
ivo://CDS.VizieR/J/A+A/293/752019-06-21T18:30:00ZJ.A_Aivo_managed1Abundances in zeta Scl open cluster (Edvardsson+, 1995)J/A+A/293/75ivo://CDS.VizieR/J/A+A/293/75CDSEDVARDSSON B., PETTERSSON B., KHARRAZI M., WESTERLUND B.[UAO]1997-12-09T17:25:4714-Jun-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frAbundancesOpen_ClustersSpectroscopy(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/293/75CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/293/75http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/293/75GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/293/75/table3Equivalent widthsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordSpeciesLine identification: chemical element and ionisation stagephys.atmol.elementLambdaWavelength0.1nmem.wlW(5)[]? Equivalent width in star No 50.1pmspect.line.eqWidthW(8)[]? Equivalent width in star No 80.1pmspect.line.eqWidthW(28)[]? Equivalent width in star No 280.1pmspect.line.eqWidthW(47)[]? Equivalent width in star No 470.1pmspect.line.eqWidthW(57)[]? Equivalent width in star No 570.1pmspect.line.eqWidthW(60)[]? Equivalent width in star No 600.1pmspect.line.eqWidthW(63)[]? Equivalent width in star No 630.1pmspect.line.eqWidthW(70)[]? Equivalent width in star No 700.1pmspect.line.eqWidthW(125)[]? Equivalent width in star No 1250.1pmspect.line.eqWidth
ivo://CDS.VizieR/J/A+A/294/1352019-06-21T18:30:00ZJ.A_Aivo_managed1Rapid variations of Eta Cen (Stefl+, 1995)J/A+A/294/135ivo://CDS.VizieR/J/A+A/294/135CDSSTEFL S., BAADE D., HARMANEC P., BALONA L.A.Patricia Bauer [CDS]1997-12-09T17:26:3231-Aug-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frSpectroscopyPhotometry:intermediate-bandStars:early-typeStars:variable(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/294/135CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/294/135http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/294/135GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/294/135/table4Photometric observations of Eta Cen obtained at the SAAO in May, 1992recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHJDHeliocentric Julian daydtime.epochymagStroemgren y magnitudemagphot.mag;em.opt.VbmagStroemgren b magnitudemagphot.mag;em.opt.BvmagStroemgren v magnitudemagphot.mag;em.opt.BumagStroemgren u magnitudemagphot.mag;em.opt.U
J/A+A/294/135/table3Photometric observations of Eta Cen obtained at the La Silla observatory in May-June, 1992recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHJDHeliocentric Julian daydtime.epochymagStroemgren y magnitudemagphot.mag;em.opt.VbmagStroemgren b magnitudemagphot.mag;em.opt.BvmagStroemgren v magnitudemagphot.mag;em.opt.BumagStroemgren u magnitudemagphot.mag;em.opt.U
J/A+A/294/135/table1Quantitative parameters measured in the Si III 455.26 nm line profiles of Eta CenrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHJDHeliocentric Julian daydtime.epochRVStellar radial velocitykm/sphys.veloc;pos.heliocentric<v>First line moment (in the heliocentric wavelength scale)km/sspect.line.width<v>cFirst line moment (in the heliocentric wavelength scale corrected for the radial velocity RVkm/sspect.line.widthFWHMFull width at half maximumkm/sspect.line.widthLDDifference of central depth of the line with respect to the mean profile (in units of 10^-3^ x continuum)phot.flux.density;arith.diffEWEquivalent width0.01nmspect.line.eqWidthymag[]? Stroemgren y magnitudemagphot.mag;em.opt.Vbmag[]? Stroemgren b magnitudemagphot.mag;em.opt.Bvmag[]? Stroemgren v magnitudemagphot.mag;em.opt.Bumag[]? Stroemgren u magnitudemagphot.mag;em.opt.Uc1[]? Stroemgren c1 colour indexmagphot.color
ivo://CDS.VizieR/J/A+A/295/1012019-06-21T18:30:00ZJ.A_Aivo_managed1Variable stars in field of NGC 7789 (Jahn+, 1995)J/A+A/295/101ivo://CDS.VizieR/J/A+A/295/101CDSJahn K., Kaluzny J., Rucinski S.M.Patricia Bauer [CDS]1997-12-09T17:26:4402-Sep-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frOpen_ClustersStars:variable(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/295/101CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/295/101http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/295/101GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/295/101/table4NGC 7789 variable starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNameName of the variablemeta.id;meta.mainHJDHeliocentric Julian daydtime.epochVmagV magnitudemagphot.mag;em.opt.Ve_Vmagrms uncertainty on Vmagstat.error
ivo://CDS.VizieR/J/A+A/296/6432019-06-21T18:30:00ZJ.A_Aivo_managed1Low Surface Brightness galaxies in Coma (Karachentsev+ 1995)J/A+A/296/643ivo://CDS.VizieR/J/A+A/296/643CDSKarachentsev I.D., Karachentseva V.E., Richter G.M., Vennik J.A.James Marcout, Patricia Bauer [CDS]1997-12-09T17:27:4007-Mar-1997CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frClusters_of_galaxiesGalaxiesUsing the prime focus of the 6-meter telescope, we have searched for low surface brightness dwarf galaxies in two regions in the Coma cluster: one in the center of the cluster and the other one 40arcmin to the west. The observations were carried out with a total exposure time 4x5x600sec and with a 1.2arcsec seeing. Our survey is complete down to V=25.5 and R=25.0mag. The central field shows an excess of faint galaxies (121 versus 104 in the reference field) significant at a one sigma level only. However, the central-field excess is mainly caused by the presence of faint (V=24/25mag), neutral colour (V-R=0.3/0.4) objects of low surface brightness, SB=26.0/26.5mag/arcsec^2^. These characteristics are quite consistent with those of the dwSph's in the Local Group which have typically M_v_~10mag and A~1kpc. The observed excess corresponds to a surface number density of 4gal/arcmin^2^ in the center of Coma, thus implying a total population of cluster dwarfs of ~4000 down to the limiting absolute magnitude -10mag. The number ratio of LSBD's to normal galaxies (with M<-18mag for normals) in Coma turns out to be 20:1. Such ratio is comparable to that observed in other rich clusters: A3574 (14:1) and A1367 (6:1), but is much larger than the 2:1 ratio obtained for moderate nearby clusters such as Virgo, Fornax, Antlia. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/296/643CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/296/643http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/296/643GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/296/643/table1Properties of galaxies in the central Coma fieldrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIDGalaxy identification numbermeta.id;meta.mainVmagApparent total V magnitudemagphot.mag;em.opt.VRmagApparent total R magnitudemagphot.mag;em.opt.RDiamVAngular diameter measured on V framearcsecphys.angSize;srcDiamRAngular diameter measured on R framearcsecphys.angSize;srcSBVAverage surface brightness within DiamVmag/arcsecphot.mag.sbSBRAverage surface brightness within DiamRmag/arcsecphot.mag.sbV-RTotal V-R color indexmagphot.color;em.opt.V;em.opt.RNoteNotes (1)meta.note
J/A+A/296/643/table2Properties of galaxies in the reference fieldrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIDGalaxy identification numbermeta.id;meta.mainVmagApparent total V magnitudemagphot.mag;em.opt.VRmagApparent total R magnitudemagphot.mag;em.opt.RDiamVAngular diameter measured on V framearcsecphys.angSize;srcDiamRAngular diameter measured on R framearcsecphys.angSize;srcSBVAverage surface brightness within DiamVmag/arcsecphot.mag.sbSBRAverage surface brightness within DiamRmag/arcsecphot.mag.sbV-RTotal V-R color indexmagphot.color;em.opt.V;em.opt.RNoteNotes (1)meta.note
ivo://CDS.VizieR/J/A+A/296/6802019-06-21T18:30:00ZJ.A_Aivo_managed1Globular Clusters Djorg 1 and Pal 6 (Ortolani+, 1995)J/A+A/296/680ivo://CDS.VizieR/J/A+A/296/680CDSORTOLANI S., BICA E., BARBUY B.Patricia Bauer [CDS]1997-12-09T17:28:1819-Sep-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frAbundancesGlobular_ClustersWe present NTT V,I observations of Palomar 6 and Djorgovski 1, two obscured loose clusters in crowded fields. We derive a reddening of E(B-V)=1.33+/-0.10, a distance d_{sun}_=~8.9kpc, and a metallicity of [Fe/H]=~-0.4 for Pal 6, and E(B-V)=1.71+/-0.10, d_{sun}_=~8.8kpc, and a similar metallicity ([Fe/H]=~-0.4) for Djorg 1. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/296/680CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/296/680http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/296/680GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/296/680/table3Djorgovski 1 datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNStellar numbermeta.id;meta.mainXX coordinatepixpos.cartesian.x;instr.detYY coordinatepixpos.cartesian.y;instr.detVmagV magnitudemagphot.mag;em.opt.VV-I(V-I) colourmagphot.color;em.opt.V;em.opt.I
J/A+A/296/680/table2Palomar 6 datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNStellar numbermeta.id;meta.mainXX coordinatepixpos.cartesian.x;instr.detYY coordinatepixpos.cartesian.y;instr.detVmagV magnitudemagphot.mag;em.opt.VV-I(V-I) colourmagphot.color;em.opt.V;em.opt.I
ivo://CDS.VizieR/J/A+A/297/282019-06-21T18:30:00ZJ.A_Aivo_managed1Dynamics in E+E pairs of galaxies (Bonfanti+, 1995)J/A+A/297/28ivo://CDS.VizieR/J/A+A/297/28CDSBONFANTI P., RAMPAZZO R., COMBES F., PRUGNIEL P., SULENTIC J.W.Patricia Bauer [CDS]1997-12-09T17:28:4720-Oct-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frGalaxies:spectraVelocitiesNGC 741/742, 1587/1588 (CPG 99) and 2672/2673 (CPG 175). All three pairs show a similar morphological distortion (i.e. the off-centering of inner versus outer isophotes; Davoust & Prugniel 1988) which is ascribed to the ongoing interaction. The data was obtained at the CFHT equipped with the Herzberg Spectrograph at a resolution of 0.88 Apx^-1^. NGC 741 and 2673 show significant rotation along the apparent minor axis. Both components of CPG 99 rotate very fast (with no evidence for rotation along the minor axis of either component). None of the galaxies show abnormally high central velocity dispersion. We report some of the first clear detections of well defined velocity dispersion curves for interacting pairs. They show a systematic decrease with distance from the center, as expected for normal ellipticals. They do not show obvious heating in the outer parts as was previously reported. NGC 741 and 2672 show, respectively, possible U and inverse U-shaped structure in their velocity profiles. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/297/28CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/297/28http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/297/28GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/297/28/table3Kinematic datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNGCNGC namemeta.id;meta.mainP.A.Position angledegpos.posAngRadiusRadiusarcsecphys.angSize;srcV(r)Velocity as function of radiuskm/sphys.veloc.rotate_V(r)rms uncertainty on V(r)km/sstat.errorsigma_V(r)[]? Velocity dispersion as function of radiuskm/sphys.veloc.dispersione_sigma_V(r)[]? rms uncertainty on sigma_Vkm/sstat.error
ivo://CDS.VizieR/J/A+A/297/3592019-06-21T18:30:00ZJ.A_Aivo_managed1Eclipsing binary HU Tauri (Parthasarathy+, 1995)J/A+A/297/359ivo://CDS.VizieR/J/A+A/297/359CDSParthasarathy M., Sarma M.B.K., Vivekananda Rao P.Patricia Bauer [CDS]1997-12-09T17:29:0017-Oct-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frBinaries:eclipsingPhotometryThe photometric elements of HU Tauri are derived from an analysis of its blue and visual light curves using the Wilson and Devinney (1971, ApJ 166, 605) light curve synthesis method. Combining the photometric elements and spectroscopic orbital elements the absolute dimensions of the system are derived. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/297/359CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/297/359http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/297/359GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/297/359/table1HU Tauri blue and yellow light curvesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordPhasephasetime.phaseDBmag[]? Differential B magnitude (HU Tau-HR 1472)magphot.mag;arith.diffDVmag[]? Differential V magnitude (HU Tau-HR 1472)magphot.mag;arith.diffNobsNumber of observations forming the normal pointsmeta.number
ivo://CDS.VizieR/J/A+A/297/492019-06-21T18:30:00ZJ.A_Aivo_managed1Supernovae spatial distribution (Petrosian+, 1995)J/A+A/297/49ivo://CDS.VizieR/J/A+A/297/49CDSPETROSIAN A.R., TURATTO M.Patricia Bauer [CDS]1997-12-09T17:29:3507-Nov-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frSuperNovaeIn order to investigate the location of supernovae (SNe) in paired and interacting galaxies, the 54 supernovae discovered up to May 1993 in 14 Isolated Pairs of Galaxies and in 32 Interacting Systems were taken as a sample and studied. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/297/49CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/297/49http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/297/49GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/297/49/table2Isolated Pairs of galaxies with SupernovaerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordGalGalaxy namemeta.id;meta.mainMTypeGalaxy typesrc.morph.typelog(Lp/Ln)[]? Logarithmic ratio of the blue luminosity of the SN parent galaxy to that of its close neighbour, corrected for galactic absorptionphys.luminosity;arith.ratioalpha[]? Far Infrared spectral index (1)spect.indexlog(LFIR/Lb)[]? Far infrared to B luminosity ratiophys.luminosity;arith.ratioD(V)[]? Difference of the velocities of the parent and the neighbour galaxy, retrieved from the most recent literaturekm/sphys.veloc;arith.diffSNSupernova namemeta.idSNTypeSupernova typesrc.classtheta[]? Distance of the SN from the center of the galaxy in units of the galactic radius at 25 mag/arcsec^2^pos.distancetheta0[]? Corrected value of theta for the tilting of the parent galaxies along the line of sightpos.distancer/R1,2[]? Ratio of the projected distance of the SN from the parent galaxy nuclei to the projected separation between components of the paired/interacting galaxiesphys.size;arith.ratioPA[]? Position angle of the SNE with respect to the neighbours (2)degpos.posAng
J/A+A/297/49/table1Interacting galaxies with supernovaerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordGalGalaxy namemeta.id;meta.mainMTypeGalaxy typesrc.morph.typelog(Lp/Ln)[]? Logarithmic ratio of the blue luminosity of the SN parent galaxy to that of its close neighbour, corrected for galactic absorptionphys.luminosity;arith.ratioalpha[]? Far Infrared spectral index (1)spect.indexlog(LFIR/Lb)[]? Far infrared to B luminosity ratiophys.luminosity;arith.ratioD(V)[]? Difference of the velocities of the parent and the neighbour galaxy, retrieved from the most recent literaturekm/sphys.veloc;arith.diffSNSupernova namemeta.idSNTypeSupernova typesrc.classtheta[]? Distance of the SN from the center of the galaxy in units of the galactic radius at 25 mag/arcsec^2^pos.distancetheta0[]? Corrected value of theta for the tilting of the parent galaxies along the line of sightpos.distancer/R1,2[]? Ratio of the projected distance of the SN from the parent galaxy nuclei to the projected separation between components of the paired/interacting galaxiesphys.size;arith.ratioPA[]? Position angle of the SNE with respect to the neighbours (2)degpos.posAng
ivo://CDS.VizieR/J/A+A/297/4942019-06-21T18:30:00ZJ.A_Aivo_managed1OH maser from semiregular variables (Szymczak+, 1995)J/A+A/297/494ivo://CDS.VizieR/J/A+A/297/494CDSSZYMCZAK M., LE SQUEREN A.M., P.SIVAGNANAM, TRAN MINH F., FOURNIER A.Patricia Bauer [CDS]1997-12-09T17:29:5020-Oct-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frMasersVelocitiesStars:variableWe have made a high sensivity (~0.15Jy) search in the OH main-lines for maser emission from a sample of 181 semiregular variables. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/297/494CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/297/494http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/297/494GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOpticalRadio
J/A+A/297/494/table2Upper limits for undetected semiregularrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIRASIRAS namemeta.idGCVSGCVS namemeta.id;meta.mainTypeType of variabilitymeta.code;src.varDateObserving date (month, year)time.epochV1Lowest velocity of the velocity rangekm/sphys.veloc;stat.minV2Highest velocity of the velocity rangekm/sphys.veloc;stat.maxn_V1[LH] L = LSR, H = heliocentricmeta.noteS1 sigma upper limit flux density (1)mJyphot.flux.density;em.radioRef[]? References (2)meta.ref
J/A+A/297/494/table1Semiregulars with OH maser emissionrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIRASIRAS namemeta.id;meta.mainGCVSGCVS namemeta.idTypeType of variabilitymeta.code;src.varDateObservation date"Y:M:D"time.epochl_Sp1(1665)limit flag on Sp1(1665)meta.code.errorSp1(1665)First peak flux density at 1665MHzJyphot.flux.density;em.radio.1500-3000MHzVp1(1665)[]? Radial velocity of Sp1(1665) (1)km/sphys.veloc;pos.heliocentricSp2(1665)[]? Second peak flux density at 1665MHzJyphot.flux.density;em.radio.1500-3000MHzVp2(1665)[]? Radial velocity of Sp2(1665) (1)km/sphys.veloc;pos.heliocentricSp3(1665)[]? Third peak flux density at 1665MHzJyphot.flux.density;em.radio.1500-3000MHzVp3(1665)[]? Radial velocity of Sp3(1665) (1)km/sphys.veloc;pos.heliocentricSp4(1665)[]? 4th peak flux density at 1665MHzJyphot.flux.density;em.radio.1500-3000MHzV4(1665)[]? Radial velocity of Sp4(1665) (1)km/sphys.veloc;pos.heliocentricSint(1665)[]? Integrated flux of the entire OH profile at 1665MHzJy.km/sphot.fluxl_Sp1(1667)limit flag on Sp1(1667)meta.code.errorSp1(1667)First peak flux density at 1667MHzJyphot.flux.density;em.radio.1500-3000MHzVp1(1667)[]? Radial velocity of Sp1(1667) (1)km/sphys.veloc;pos.heliocentricSp2(1667)[]? Second peak flux density at 1667MHzJyphot.flux.density;em.radio.1500-3000MHzVp2(1667)[]? Radial velocity of Sp2(1667) (1)km/sphys.veloc;pos.heliocentricSint(1667)[]? Integrated flux of the entire OH profile at 1667MHzJy.km/sphot.fluxNotesNotes (2)meta.note
ivo://CDS.VizieR/J/A+A/297/5032019-06-21T18:30:00ZJ.A_Aivo_managed1HD 146850 (Castilho+, 1995)J/A+A/297/503ivo://CDS.VizieR/J/A+A/297/503CDSCASTILHO B.V., BARBUY B., GREGORIO-HETEM J.Patricia Bauer [CDS]1997-12-09T17:30:0220-Sep-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frStarsSpectroscopyWe report the identification of 3 Li-rich giants discovered in an ongoing survey based on IRAS colours. A detailed analysis of one of these, HD 146850, is presented here. High resolution spectra were obtained for this star, using CASPEC at the 3.6m telescope of ESO. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/297/503CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/297/503http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/297/503GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/297/503/table2DatarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordLamWavelength0.1nmem.wlElementElementphys.atmol.elementIonIonisation stagephys.atmol.ionizationExcExcitation potentialeVphys.energy;phys.atmol.excitationlog(gf)Oscillator strengthphys.atmol.wOscStrengthWEquivalent width0.1pmspect.line.eqWidth
ivo://CDS.VizieR/J/A+A/297/612019-06-21T18:30:00ZJ.A_Aivo_managed1E+A galaxies in Cl0939+472 (Belloni+, 1995)J/A+A/297/61ivo://CDS.VizieR/J/A+A/297/61CDSBELLONI P., BRUZUAL A.G., THIMM G.J.,ROESER H.-J.Patricia Bauer [CDS]1997-12-09T17:30:1508-Nov-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frClusters_of_galaxiesPhotometryWe present results of a study of E+A galaxies in the cluster Cl0939+472 (z=0.41). We have used a series of narrow-band filters (FWHM~=90-200A) covering the range from 3800 to 9200A, and broad band B, R, I filters to obtain low resolution spectra for all galaxies brighter than R=22.5mag in a 5'x5' cluster field. Two of the narrow-band filters have been chosen to measure the 4000A-break index, and 3 filters were centered on the H_{beta}_, H_{gamma}_ and H_{delta}_ lines which are indicators of recent star formation. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/297/61CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/297/61http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/297/61GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/297/61/table8E+A galaxies in Cl0939+472recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIDIdentification numbermeta.id;meta.mainxposx position (1)arcsecpos.cartesianyposy position (1)arcsecpos.cartesianRmagR magnitudemagphot.mag;em.opt.RB-RB-R colourmagphot.color;em.opt.B;em.opt.RB-IB-I colourmagphot.color;em.opt.B;em.opt.ID4000D4000 index (4000 A-break) (2)spect.indexzD[]? Redshift for DGsrc.redshiftzRedshifth derived from this worksrc.redshifte_z1-sigma error on zstat.errorAgeGalaxy age after the beginning of the second starburstMyrtime.ageMType(HST)Morphology type derived from Hubble Space Telescope (HST)src.morph.type
J/A+A/297/61/table9Redshifts and morphological type for all objects that could be identified in Dressler A., 1992, STScI Newsletter 9, 2.recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIDIdentification numbermeta.id;meta.mainzD[]? Redshift derived from DGsrc.redshiftzRedshift derived from this worksrc.redshifte_z1-sigma error on zstat.errorMType(SED)Morphology type derived from spectral energy distribution (SED)src.morph.typeMType(HST)Morphology type derived from Hubble Space Telescope (HST)src.morph.type
ivo://CDS.VizieR/J/A+A/299/2382019-06-21T18:30:00ZJ.A_Aivo_managed1Radio observations of PN candidates (Van de Steene+, 1995)J/A+A/299/238ivo://CDS.VizieR/J/A+A/299/238CDSVAN DE STEENE G.C., POTTASCH S.R.Patricia Bauer [CDS]1997-12-09T17:31:4016-Jan-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frWe analyzed radio continuum observations of unidentified IRAS point sources with far IR colors that are typical of planetary nebulae. These IRAS-selected planetary nebula candidates are located outside the galactic bulge and were observed with the Westerbork Radio Synthesis Telescope. We have detected 20 new planetary nebulae out of 82 observed candidates. The detected sources are very close to the galactic plane. The detection rate is highest in that part of the color-color diagram, where planetary nebulae are expected to spend most time during their evolution. The radio and IR properties are compared with PN detected in the same way in the galactic bulge and with optical planetary nebulae which fulfill the same selection criteria. On average, the IR excess of the IRAS-selected and radio detected planetary nebula candidates is higher than for the optical planetary nebulae. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/299/238CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/299/238http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/299/238GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table J/A+A/299/238/table1 (Far infrared data of the observed PN candidates in WSRT1 (Westerbork Synthesis Radio Telescope))http://vizier.u-strasbg.fr/viz-bin/conesearch/J/A+A/299/238/table1?GETtext/xml+votable18050000true67.5659179687535.961364378928390.028629053431811713Cone search capability for table J/A+A/299/238/table3 (Far infrared data of the observed PN candidates in WSRT2)http://vizier.u-strasbg.fr/viz-bin/conesearch/J/A+A/299/238/table3?GETtext/xml+votable18050000true70.3344726562528.673496936394410.028629053431811713Radiohttp://alasky.u-strasbg.fr/footprints/cats/vizier/J/A+A/299/238?product=MOC&nside=512
J/A+A/299/238/table1Far infrared data of the observed PN candidates in WSRT1 (Westerbork Synthesis Radio Telescope)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIdSequential numbermeta.id;meta.mainRA1950Right ascension 1950.0"h:m:s"pos.eq.ra;meta.mainDE1950Declination sign"d:m:s"pos.eq.dec;meta.mainGLON[-178.2,172.0] Galactic longitudedegpos.galactic.lonGLATGalactic latitudedegpos.galactic.latF12Far IR flux density at 12 {mu}mJyphot.flux.density;em.IR.8-15umF25Far IR flux density at 25 {mu}m (upper limit for table3)Jyphot.flux.density;em.IR.15-30umF60Far IR flux density at 60 {mu}mJyphot.flux.density;em.IR.30-60umF100Far IR flux density at 100 {mu}mJyphot.flux.density;em.IR.60-100umq_F12Quality of F12 (1)meta.code.qualq_F25Quality of F25 (1)meta.code.qualq_F60Quality of F60 (1)meta.code.qualq_F100Quality of F100 (1)meta.code.qualF12/F25IRAS colour F12/F25phot.color;em.IR;em.IRF25/F60IRAS colour F25/F60phot.color;em.IR;em.IRTcColor temperatureKphys.temperatureFIRTotal far infrared flux10-13W/m2phot.flux;em.IRrmsrms error of the values of the fitted black body curve at 12, 25 and 60 {mu}m compared with the IRAS flux values at these wavelengths respectivelyJystat.error
J/A+A/299/238/table3Far infrared data of the observed PN candidates in WSRT2recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIdSequential numbermeta.id;meta.mainRA1950Right ascension 1950.0"h:m:s"pos.eq.ra;meta.mainDE1950Declination sign"d:m:s"pos.eq.dec;meta.mainGLON[-178.2,172.0] Galactic longitudedegpos.galactic.lonGLATGalactic latitudedegpos.galactic.latF12Far IR flux density at 12 {mu}mJyphot.flux.density;em.IR.8-15umF25Far IR flux density at 25 {mu}m (upper limit for table3)Jyphot.flux.density;em.IR.15-30umF60Far IR flux density at 60 {mu}mJyphot.flux.density;em.IR.30-60umF100Far IR flux density at 100 {mu}mJyphot.flux.density;em.IR.60-100umq_F12Quality of F12 (1)meta.code.qualq_F25Quality of F25 (1)meta.code.qualq_F60Quality of F60 (1)meta.code.qualq_F100Quality of F100 (1)meta.code.qualF12/F25IRAS colour F12/F25phot.color;em.IR;em.IRF25/F60IRAS colour F25/F60phot.color;em.IR;em.IRTcColor temperatureKphys.temperatureFIRTotal far infrared flux10-13W/m2phot.flux;em.IRrmsrms error of the values of the fitted black body curve at 12, 25 and 60 {mu}m compared with the IRAS flux values at these wavelengths respectivelyJystat.error
ivo://CDS.VizieR/J/A+A/299/4532019-06-21T18:30:00ZJ.A_Aivo_managed1OH/IR stars photometry (Lepine+, 1995)J/A+A/299/453ivo://CDS.VizieR/J/A+A/299/453CDSLEPINE J.R.D., ORTIZ R., EPCHTEIN N.Patricia Bauer [CDS]1997-12-09T17:32:1321-Feb-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frMasersThis paper presents JHKL'M photometry of a new sample of OH/IR stars. These data are merged with similar observations collected in the literature in order to constitute a data base of near-infrared photometry for 400 OH/IR stars. After removing from this sample the objects that are unlikely to be AGB stars, we obtain a sequence of average OH/IR stars with increasing values of the colour index K-L'. A simple model of a star surrounded by a circumstellar shell is constructed in order to derive basic parameters such as luminosity, radius, stellar temperature, optical depth of the dust shell and mass loss rate. These parameters are found to vary smoothly along the sequence of OH/IR stars, and the K-L' colour is shown to describe almost completely the basic physical parameters of an OH/IR star. The metallicity affects the OH-peak separation, but does not play an important role in the definition of the other properties. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/299/453CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/299/453http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/299/453GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapInfraredRadio
J/A+A/299/453/table2Catalog of near-infrared photometry of OH/IR starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIRASIRAS namemeta.id;meta.mainm_IRASMultiplicity index on IRASmeta.code.multipLONLongitudedegpos.earth.lonLATLatitudedegpos.earth.latVlowLowest velocitykm/sphys.veloc;pos.heliocentricVhighHighest velocitykm/sphys.veloc;pos.heliocentricDistDistancekpcpos.distanceKmagK magnitudemagphot.mag;em.IR.KJ-H[]? J-H colourmagphot.color;em.IR.J;em.IR.HH-K[]? H-K colourmagphot.color;em.IR.H;em.IR.KK-L[]? K-L colourmagphot.color;em.IR.K;em.IR.3-4umL-M[]? L-M colourmagphot.color;em.IR.3-4um;em.IR.4-8um
J/A+A/299/453/table1Near-infrared counterparts of OH/IR starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIRASIRAS namemeta.id;meta.mainRefReference (1)meta.refOtherRefOther reference (1)meta.ref
ivo://CDS.VizieR/J/A+A/299/532019-06-21T18:30:00ZJ.A_Aivo_managed1Red giants in NGC 3680 and IC 4651 (Mermilliod+, 1995)J/A+A/299/53ivo://CDS.VizieR/J/A+A/299/53CDSMERMILLIOD J.-C., ANDERSEN J., NORDSTROM B., MAYOR M.Patricia Bauer [CDS]1997-12-09T17:32:3013-Feb-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frOpen_ClustersStarsVelocities(no description available) http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/299/53CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/299/53http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/299/53GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/299/53/n3680Radial velocity data for NGC 3680recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIDStar number (1)meta.id;meta.mainHJDHeliocentric Julian Datedtime.epochCompComponent of a double-lined binarymeta.noteRVRadial velocitykm/sphys.veloc;pos.heliocentrice_RVrms uncertainty on the radial velocitykm/sstat.error
J/A+A/299/53/i4651Radial velocity data for IC 4651recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIDStar number (1)meta.id;meta.mainHJDHeliocentric Julian Datedtime.epochCompComponent of a double-lined binarymeta.noteRVRadial velocitykm/sphys.veloc;pos.heliocentrice_RVrms uncertainty on the radial velocitykm/sstat.error
ivo://CDS.VizieR/J/A+A/299/5572019-06-21T18:30:00ZJ.A_Aivo_managed1Light variations on Beta Pic (Lecavelier des Etangs+, 1995)J/A+A/299/557ivo://CDS.VizieR/J/A+A/299/557CDSLECAVELIER DES ETANGS A., DELEUILE M., VIDAL-MADJAR A., FERLET R. NITSCHLEM C., NICOLET B., LAGRANGE-HENRI A.M.Simona Mei, Patricia Bauer [CDS]1997-12-09T17:32:4521-Feb-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frStarsPhotometry:wide-bandWe have analyzed {beta} Pictoris photometric measurements obtained from La Silla by the Geneva Observatory from 1975 to 1992. These data show evidence of variations in the brightness of the star, with no color dependency. Here, we demonstrate that the light variations are present on long as well as on short time scales. On a long time scale, we show that the apparent magnitude of {beta} Pictoris decreased by 0.011+/-0.004mag from 1979 to 1982. Moreover, when we consider all the measurements, the chance that there is no variation at all can be estimated to be less than 10^-4^. On short time scales there is a peculiar feature observed during about 30 days; the variations may be as high as 0.04mag magnitude. A maximum entropy reconstruction of the photometric data is tentatively proposed and some physical interpretations are presented. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/299/557CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/299/557http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/299/557GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/299/557/tableGeneva photometryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordJDJulian datedtime.epochq_VmagQuality factor of the V magnitudemeta.code.qualVmagV magnitudemagphot.mag;em.opt.Vq_coloursQuality factor of the colour indexesmeta.code.qualU-BU-B colour indexmagphot.colorV-BV-B colour indexmagphot.colorB1-BB1-B colour indexmagphot.colorB2-BB2-B colour indexmagphot.colorV1-BV1-B colour indexmagphot.colorG-BG-B colour indexmagphot.color
ivo://CDS.VizieR/J/A+A/299/6212019-06-21T18:30:00ZJ.A_Aivo_managed1Is Sirius a triple star? (Benest+, 1995)J/A+A/299/621ivo://CDS.VizieR/J/A+A/299/621CDSBENEST D., DUVENT J.L.Patricia Bauer [CDS]1997-12-09T17:33:0428-Nov-1994CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frOrbitsStarsSirius has been discovered as double more than 130 years ago. From the beginning of our century up to now, observational as well as physical and dynamical indications lead to the hypothesis of the existence of a third body in the system. In this paper, we present recent orbital analysis of the binary Sirius A-B which, helped by numerical simulation of triple systems, strengthens the idea for the triplicity of Sirius: a tiny star could revolve in about 6 years around Sirius A. Finally, we discuss the possibility of direct detection for this suspected Sirius C. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/299/621CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/299/621http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/299/621GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tap
J/A+A/299/621/table2Mean square Fourier analysisrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordPPeriodyrtime.periodAxFourier transforms Ax of O-Cxstat.paramAyFourier transforms Ay of O-Cystat.paramAxyMean of Ax, Aystat.param
J/A+A/299/621/appenObservations of Sirius (1862-1979)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordDateObservation dateyrtime.epochThetaPosition angledegpos.posAngu_Theta[?)] Uncertainty flag on Thetameta.code.errorRhoSeparation anglearcsecpos.angDistanceu_Rho[?)] Uncertainty flag on Rhometa.code.erroro_ThetaNumber of observationsmeta.numberNameObserver name (1)obs.observer
J/A+A/299/621/table3Mean square sine function analysis (all data)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordPPeriodyrtime.periodAxPerturbation amplitude Ax of O-Cxstat.paramAyPerturbation amplitude Ay of O-Cystat.paramAxyMean of Ax, Aystat.param
ivo://CDS.VizieR/J/A+A/299/6962019-06-21T18:30:00ZJ.A_Aivo_managed1Pleiades field Membership probabilities (Schilbach+, 1995)J/A+A/299/696ivo://CDS.VizieR/J/A+A/299/696CDSSCHILBACH E., ROBICHON N., SOUCHAY J., GUIBERT J.Simona Mei [CDS]1997-12-09T17:33:2121-Feb-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frOpen_ClustersPhotometryProper_MotionsA catalogue of proper motions and photographic B,V magnitudes for stars up to B=19 mag within a region centered near Alcyone is presented. The catalogue is based on MAMA measurements of 8 plates taken with the Tautenburg Schmidt telescope. The survey includes ca. 14500 stars and covers a total field of about 9 square degrees. Membership probabilities, proper motions and B,V magnitudes are listed for 442 stars up to B=19 mag in the Pleiades field. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/299/696CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/299/696http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/299/696GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapCone search capability for table J/A+A/299/696/table1 (Position, proper motions, photometry and membership probabilities.)http://vizier.u-strasbg.fr/viz-bin/conesearch/J/A+A/299/696/table1?GETtext/xml+votable18050000true57.5903320312523.1150132779652750.028629053431811713Opticalhttp://alasky.u-strasbg.fr/footprints/cats/vizier/J/A+A/299/696?product=MOC&nside=512
J/A+A/299/696/table1Position, proper motions, photometry and membership probabilities.recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIndexIdentification indexmeta.id;meta.mainn_IndexSee (1)meta.noteRAJ2000Right ascension (Eq. J2000.0, Ep. 1981.1)"h:m:s"pos.eq.ra;meta.mainDEJ2000Declination (Eq. J2000.0, Ep. 1981.1)"d:m:s"pos.eq.dec;meta.mainpmRAProper motion in right ascensionmas/yrpos.pm;pos.eq.rae_pmRARms uncertainty on pmRAmas/yrstat.errorpmDEProper motion in declinationmas/yrpos.pm;pos.eq.dece_pmDERms uncertainty on pmDEmas/yrstat.errorBmagMagnitude Bmagphot.mag;em.opt.BVmagMagnitude Vmagphot.mag;em.opt.VprobMembership probability%stat.fit.goodnessNameOther name (2)meta.id
ivo://CDS.VizieR/J/A+A/300/1282019-06-21T18:30:00ZJ.A_Aivo_managed1ESO 96-SC04 and ESO 92-SC18 photometry (Carraro+, 1995)J/A+A/300/128ivo://CDS.VizieR/J/A+A/300/128CDSCARRARO G., VALLENARI A., ORTOLANI S.Patricia Bauer, Francois Ochsenbein [CDS]1997-12-09T17:34:1021-Feb-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frOpen_ClustersPhotometryWe present deep CCD BV photometry in the central region of the faint open clusters ESO 96-SC04 and ESO 92-SC18. The color magnitude diagrams (CMD) here presented allows us to evaluate the clusters ages. We found an age of 5.0x10^9^yr for ESO 92-SC18 and 0.7x10^9^yr for ESO 96-SC04 on the Padova isochrones scale. Estimates of the reddening are given for both the target clusters and the distances of these objects are substantially revised. We conclude that these clusters belong to the old tail of the thin disk population, they are among the most distant known open clusters from the Sun and lie near the solar circle like the majority of the open clusters. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/300/128CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/300/128http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/300/128GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/300/128/eso92ESO 92-SC18 photometryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordSeq[]+ Star identification (running) numbermeta.id;meta.mainXposX coordinatepixpos.cartesian.x;instr.detYposY coordinatepixpos.cartesian.y;instr.detVmagV magnitudemagphot.mag;em.opt.VB-VB-V colourmagphot.color;em.opt.B;em.opt.V
J/A+A/300/128/eso96ESO 96-SC04 photometryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordSeq[]+ Star identification (running) numbermeta.id;meta.mainXposX coordinatepixpos.cartesian.x;instr.detYposY coordinatepixpos.cartesian.y;instr.detVmagV magnitudemagphot.mag;em.opt.VB-VB-V colourmagphot.color;em.opt.B;em.opt.V
ivo://CDS.VizieR/J/A+A/300/7262019-06-21T18:30:00ZJ.A_Aivo_managed1BH 176 and AM-2 (Ortolani+, 1995)J/A+A/300/726ivo://CDS.VizieR/J/A+A/300/726CDSORTOLANI S., BICA E., BARBUY B.Patricia Bauer [CDS]1997-12-09T17:34:4906-Jan-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frGlobular_ClustersOpen_ClustersPhotometryWe have obtained VI photometry for two low Galactic latitude star clusters: BH 176 and AM-2, using the 2.2m and the 3.5m NTT telescopes at ESO. Their VI colour-magnitude diagrams reveal that: BH 176 may be a globular cluster, or a border line object between a globular cluster and a disk cluster, showing a red horizontal branch and an extended red giant branch. We estimate E(B-V)=0.77 and d_{sun}_=13.4kpc. AM-2 appears to be an intermediate age open cluster, for which a reddening E(B-V)=0.44 and d_{sun}_=12.4kpc are estimated. It is located in the outer regions of the Galactic disk. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/300/726CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/300/726http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/300/726GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/300/726/table3BH 176 coordinates, V magnitude and V-I colourrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNoStar numbermeta.id;meta.mainXX coordinatepixpos.cartesian.x;instr.detYY coordinatepixpos.cartesian.y;instr.detVmagV magnitudemagphot.mag;em.opt.VV-I(V-I) colourmagphot.color;em.opt.V;em.opt.I
J/A+A/300/726/table2AM-2 coordinates, V magnitude and V-I colourrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNoStar numbermeta.id;meta.mainXX coordinatepixpos.cartesian.x;instr.detYY coordinatepixpos.cartesian.y;instr.detVmagV magnitudemagphot.mag;em.opt.VV-I(V-I) colourmagphot.color;em.opt.V;em.opt.I
ivo://CDS.VizieR/J/A+A/301/3962019-06-21T18:30:00ZJ.A_Aivo_managed1Photometry of NGC 1962-65-66-70 (Will J.-M.+, 1995)J/A+A/301/396ivo://CDS.VizieR/J/A+A/301/396CDSWILL J.M., VAZQUEZ A., FEINSTEIN A., SEGEEWISS W.Simona Mei [CDS]1997-12-09T17:35:2603-Apr-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frAssociationsPhotometry:wide-bandWe present CCD data in the Johnson passbands B and V of the young association NGC 1962-65-66-70 in the Large Magellanic Cloud. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/301/396CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/301/396http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/301/396GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/301/396/table3Photometry of 1920 stars in the field of NGC 1962-65-66-70 in the B and V passbands.recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordStarStar running numbermeta.id;meta.mainXposposition on CCD frame as given by DAOPHOTpixpos.cartesian.x;instr.detYposposition on CCD frame as given by DAOPHOTpixpos.cartesian.y;instr.detVmagCalibrated V magnitude of starmagphot.mag;em.opt.VB-VCalibrated B-V colour of starmagphot.color;em.opt.B;em.opt.Ve_VmagRms uncertainty on V magnitudemagstat.errore_B-VRms uncertainty on B-V colourmagstat.error
ivo://CDS.VizieR/J/A+A/303/1752019-06-21T18:30:00ZJ.A_Aivo_managed1Line spectrum of NGC 7027 (Baluteau+, 1995)J/A+A/303/175ivo://CDS.VizieR/J/A+A/303/175CDSBALUTEAU J.-P., ZAVAGNO A., MORISSET C., PEQUIGNOT D.Patricia Bauer [CDS]1997-12-09T17:35:5307-Mar-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frSpectroscopyDeep CCD spectra of the planetary nebula NGC 7027, taken over the range 654-1046nm at a spectral resolution of the order of 0.1nm, are presented. About 465 different lines are detected and intensities are provided for 405 features. A total of 680 emission lines is considered. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/303/175CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/303/175http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/303/175GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/303/175/table2Lines in the spectrum of NGC 7027recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordIdLine identification (1)meta.idLamTheo[]? Theoretical wavelengthnmem.wl;phys.atmol.transitionn_LamTheo[}*] '}' indicates several identification lines for the same observed wavelength '*' indicates a note on [FeIV]meta.noteu_LamTheo[?] Uncertainty flag on LamTheometa.code.errorLamObsObserved wavelengthnmem.wlo_LamObs[]? Number of independent measurementsmeta.numberIlam/Ibeta[]? Line intensity in I(Hbeta)/10+410-4spect.line.intensity;arith.ratioe_Ilam/Ibeta[]? rms uncertainty on 10+4F/Ibeta%stat.errorComComments (2)meta.note
ivo://CDS.VizieR/J/A+A/303/4682019-06-21T18:30:00ZJ.A_Aivo_managed1Spectrospcopy, IR-photom. in globular clusters (Minniti, 1995)J/A+A/303/468ivo://CDS.VizieR/J/A+A/303/468CDSMinniti D.Patricia Bauer [CDS]1997-12-09T17:36:2102-Feb-1996CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frSpectroscopyVelocitiesWe have obtained spectra of 85 giants selected from IR photometry in the fields of several very reddened galactic clusters. Radial velocities are measured to check membership. We measure the strength of several Fe and Mg spectral feature s, presenting a new calibration of metallicity based on the location of the giants in the Mg+Fe5270+Fe5335 vs (J-K)_0_ diagram. Using this calibration we compute accurate mean metallicities for the clusters studied. Reddening values which better fit the spectroscopic and photometric data are also derived. Pal 6 turns out to be the most metal rich cluster of our sample, with [Fe/H]=0.2+/-0.3. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/303/468CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/303/468http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/303/468GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapInfrared
J/A+A/303/468/table3Colors, velocities and spectral indicesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordClusterCluster namemeta.id.part;meta.mainStarStar namemeta.id.part;meta.mainJ-K? Measured J-K colourmagphot.color;em.IR.J;em.IR.KRV? Measured heliocentric radial velocitykm/sphys.veloc;pos.heliocentricMgMg spectroscopic index (1)spect.indexHbetaHbeta spectroscopic index (1)spect.index;em.line.HbetaFe492Fe492 spectroscopic index (1)spect.indexFe498Fe498 spectroscopic index (1)spect.indexFe501Fe501 spectroscopic index (1)spect.indexFe527Fe527 spectroscopic index (1)spect.indexFe533Fe533 spectroscopic index (1)spect.indexFe540Fe540 spectroscopic index (1)spect.indexMg1Mg1 spectroscopic index (1)spect.indexMg2Mg2 spectroscopic index (1)spect.indexMgbMgb spectroscopic index (1)spect.indexMgHMgH spectroscopic index (1)spect.index
ivo://CDS.VizieR/J/A+A/303/8932019-06-21T18:30:00ZJ.A_Aivo_managed1Planetary nebulae with WR-type nuclei (Gorny+, 1995)J/A+A/303/893ivo://CDS.VizieR/J/A+A/303/893CDSGORNY S.K., STASINSKA G.Simona Mei [CDS]1997-12-09T17:36:4515-May-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frStars:WRA recent systematic search of Wolf-Rayet features in the spectra of Galactic planetary nebulae has increased the list of objects that are known to have WR-type nuclei to about 50. We have compared their nebular properties with those of the other planetary nebulae in the Galaxy. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/303/893CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/303/893http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/303/893GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/303/893/table2Morphological types of the non-WR planetary nebulaerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordPNGPNG designationmeta.id;meta.mainNameNamemeta.idMtypeMorphological typesrc.morph.typeRefSouReferences to images sources (1)meta.ref
J/A+A/303/893/table1Properties of planetary nebulae with WR-type central starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordPNGPNG designationmeta.id;meta.mainNameNamemeta.idSpSpectral class of the central starsrc.spTypeMTypeMorphological type (1)src.morph.typeRefSouReferences to images sources (2)meta.refl_He/HUpper/lower He/H ratio limit signmeta.code.errorHe/H[]? He/H abundance ratiophys.abundu_He/HHe/H ratio uncertainty flagmeta.code.errorN/O[]? N/O abundance ratiophys.abundu_N/ON/O ratio uncertainty flagmeta.code.errorC/O[]? C/O abundance ratiophys.abundu_C/OC/O ratio uncertainty flagmeta.code.errorRefAbunReference to abundances (2)phys.abundExpVel[]? 2*expansion velocitykm/sphys.veloc.expansionu_ExpVelExpansion velocity uncertainty flagmeta.code.errorr_ExpVelReference to expansion velocity (2)meta.refMLRate[]? Mass loss rate10-6solMass/yrphys.mass.lossr_MLRateReference to mass loss rate (2)meta.ref
ivo://CDS.VizieR/J/A+A/304/2352019-06-21T18:30:00ZJ.A_Aivo_managed1UBV Photometry of phi Per (Bozic+, 1995)J/A+A/304/235ivo://CDS.VizieR/J/A+A/304/235CDSBozic H., Harmanec P., Horn J., Koubsky P., Scholz G., McDavid D., Hubert A.-M., Hubert H.Simona Mei [CDS]1997-12-09T17:36:5815-May-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometry:wide-bandStars:variableA detailed analysis of a very rich collection of spectroscopic and photometric observations of the bright Be star {phi} Per (HR 496, or HD 10516, 2000 position: 01 43 39.4 +50 41 20) is presented. Earlier reports that {phi} Per is a double-lined spectroscopic binary consisting of two emission-line objects are confirmed. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/304/235CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/304/235http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/304/235GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/304/235/table6aUBV photometry of Phi PerrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHJDJulian datedtime.epochWeightWeightstat.weightVmag[]? V magnitudemagphot.mag;em.opt.Ve_Vmag[]? rms uncertainty on V magnitudemagstat.errorBmag[]? B magnitudemagphot.mag;em.opt.Be_Bmag[]? rms uncertainty on B magnitudemagstat.errorUmag[]? U magnitudemagphot.mag;em.opt.Ue_Umag[]? rms uncertainty on U magnitudemagstat.errorB-V[]? B-V colour indexmagphot.color;em.opt.B;em.opt.VU-B[]? U-B colour indexmagphot.color;em.opt.U;em.opt.BStationObserving station and instruments (1)meta.id;instr.obsty
J/A+A/304/235/table6bAll-sky UBV photometry of Phi PerrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordHJDJulian datedtime.epochWeightWeightstat.weightVmag[]? V magnitudemagphot.mag;em.opt.Ve_Vmag[]? rms uncertainty on V magnitudemagstat.errorBmag[]? B magnitudemagphot.mag;em.opt.Be_Bmag[]? rms uncertainty on B magnitudemagstat.errorUmag[]? U magnitudemagphot.mag;em.opt.Ue_Umag[]? rms uncertainty on U magnitudemagstat.errorB-V[]? B-V colour indexmagphot.color;em.opt.B;em.opt.VU-B[]? U-B colour indexmagphot.color;em.opt.U;em.opt.BStationObserving station and instruments (1)meta.id;instr.obsty
ivo://CDS.VizieR/J/A+A/304/4062019-06-21T18:30:00ZJ.A_Aivo_managed1Photometry and radial velocities of 16 Lac (Chapellier+, 1995)J/A+A/304/406ivo://CDS.VizieR/J/A+A/304/406CDSChapellier E., Le Contel J.M., Le Contel D., Sareyan J.P., Valtier J.C.Simona Mei [CDS]1997-12-09T17:37:5407-Jun-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frPhotometryVelocitiesStars:variablePhotometric and spectroscopic observations of the {beta} Cephei star 16 Lacertae obtained in 1983 and 1984 are presented and analysed. Using all the published maxima we have computed ephemerides for each of the three pulsational modes. No period variation is detected from 1950 to 1983. In order to identify the pulsational modes corresponding to the three main periods of 16 Lac we have applied different methods based on photometric and radial velocity variations. All give the same results: the mode corresponding to the largest amplitude P_1_ (016917d) is radial, P_2_ (017079d) is a nonradial mode of degree l=2. For P_3_ (018171d) the results are more dubious, but P_3_ is probably a l=1 nonradial mode. We have also studied the interaction between pulsation and binarity in 16 Lac. We confirm the existence of a resonance phenomenon between the radial and nonradial modes: the ratios between the beat frequencies of the pulsational modes and the orbital frequency are close but significantly different from simple rational numbers. According to Kato (1974) that means that the nonradial modes might be excited or at least enhanced by tidal effects. They would have been selected among all the possible modes because their ability to be resonant with the radial mode. The photometric amplitude of P_3_ in both filters appears to be variable from night to night in correlation with the orbital phase but despite its rapid and irregular fluctuations, the P_3_ amplitude stayed in constant average over 80 years. The present observations confirm the decrease of P_1_ and P_2_ amplitudes since 1950 but an analysis of older radial velocity data shows that the amplitude of the P_1_ mode went through a maximum around the middle of the century before the observed decrease of the last thirty years. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/304/406CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/304/406http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/304/406GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/304/406/photoPhotometric datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordDateDate"Y:M:D"time.epochFilter[4,5] Filter (1)meta.code;instr.filterJDJulian daydtime.epochDMagMagnitude difference between 16 Lac and 2 Andmagphot.mag;arith.diff
J/A+A/304/406/veloRadial velocity datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordJDJulian daydtime.epochRVRadial velocity of 16 Lac.km/sphys.veloc;pos.heliocentric
ivo://CDS.VizieR/J/A+A/304/4152019-06-21T18:30:00ZJ.A_Aivo_managed1uvby-Hbeta photometry of Eta Car 1992-94 (van Genderen+, 1995)J/A+A/304/415ivo://CDS.VizieR/J/A+A/304/415CDSvan Genderen A.M., Sterken C., de Groot M., Stahl O., Andersen J., Andersen M.I., Caldwell J.A.R., Casey B., Clement R., Corradi W.J.B., Cuypers J., Debehogne H., Garcia de Maria J.M., Joench-Soerensen H., Vaz L.P.R., Stefl S., Suso Lopez J., Beele D., EgSimona Mei [CDS]1997-12-09T17:38:0626-Jul-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frStarsPhotometry:intermediate-bandStars:variableWe present and analyze two seasons of intense photometric monitoring in the Stroemgren uvbyH{beta} system of {eta} Carinae (October 1992-August 1994). The luminous blue variable (LBV) in the core did not show much S Dor activity, i.e. it was in a relatively quiescent stage. This situation was very favourable for studying its optical micro variations. It appears that the central LBV pulsates (presumably in a non-radial mode) like other massive evolved stars, the {alpha} Cyg variables. The quasi-period is 58.56d. The linear ephemeris is: JD_max_=2448875.0 +58.56 E. Support was found for the existence of the presumed periodicity of 52.4d of the so-called "dimples", shallow dips in the light curve which only last for a few days. The cause may be the eclipse of a small companion or of a hot spot in an accretion disk. The H{beta} index became bluer by ~0.07mag during the last 11/2 years and shows an oscillation in anti-phase with the 58.56d pulsation, suggesting that the HII region(s) responsible for the hydrogen line emission has a relatively high luminosity. This is another reason to suppose that a second luminous source, perhaps a luminous disk (with a hot spot), may be present in the {eta} Car system. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/304/415CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/304/415http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/304/415GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/304/415/table1Stroemgren uvbyH-beta photometry of Eta CarrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordJDJulian datedtime.epochu_JD[:] Uncertainty flag on JDmeta.code.errorymag[]? y Stroemgren magnitudemagphot.mag;em.opt.Vbmag[]? b Stroemgren magnitudemagphot.mag;em.opt.Bvmag[]? v Stroemgren magnitudemagphot.mag;em.opt.Bumag[]? u Stroemgren magnitudemagphot.mag;em.opt.UHbmag[]? H{beta} Stroemgren magnitudemagspect.index
ivo://CDS.VizieR/J/A+A/305/2452019-06-21T18:30:00ZJ.A_Aivo_managed1Fe I in metal-poor stars (Magain+, 1996)J/A+A/305/245ivo://CDS.VizieR/J/A+A/305/245CDSMagain P., Zhao G.Simona Mei [CDS]1997-12-09T17:38:1807-Jun-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frAbundancesEquivalent_widthsA detailed analysis of neutral iron lines in a sample of 13 metal-poor dwarfs and subgiants is carried out on the basis of high resolution spectra obtained with the ESO Coude Echelle Spectrometer. The deduced iron abundance is found to depend on the excitation potential of the line used, higher excitation lines generally indicating higher abundances. This could be caused by departures from the local thermodynamic equilibrium (LTE) or by temperature inhomogeneities in the stellar atmospheres. The dependency of this effect on the stellar atmospheric parameters is investigated. From the comparison of iron lines with lines of other elements, it is concluded that the low excitation Fe I lines are much more affected than the high excitation lines. The consequences of these effects for the classical abundance analyses are examined. It is found that they may explain, at least in part, some previously reported discrepancies between the results of different authors. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/305/245CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/305/245http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/305/245GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOptical
J/A+A/305/245/table4Equivalent widths and abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordElementElementphys.atmol.elementLambdaLine wavelength0.1nmem.wlEW3567[]? Equivalent width for the star HD 35670.1pmspect.line.eqWidthAb3567[]? Abundance for the star HD 3567 (1)phys.abundEW25704[]? Equivalent width for the star HD 257040.1pmspect.line.eqWidthAb25704[]? Abundance for the star HD 25704 (1)phys.abundEW122196[]? Equivalent width for the star HD 1221960.1pmspect.line.eqWidthAb122196[]? Abundance for the star HD 122196 (1)phys.abundEW126793[]? Equivalent width for the star HD 1267930.1pmspect.line.eqWidthAb126793[]? Abundance for the star HD 126793 (1)phys.abundEW132475[]? Equivalent width for the star HD 1324750.1pmspect.line.eqWidthAb132475[]? Abundance for the star HD 132475 (1)phys.abundEW152924[]? Equivalent width for the star HD 1529240.1pmspect.line.eqWidthAb152924[]? Abundance for the star HD 152924 (1)phys.abundEW160617[]? Equivalent width for the star HD 1606170.1pmspect.line.eqWidthAb160617[]? Abundance for the star HD 160617 (1)phys.abundEW166913[]? Equivalent width for the star HD 1669130.1pmspect.line.eqWidthAb166913[]? Abundance for the star HD 166913 (1)phys.abundEW189558[]? Equivalent width for the star HD 1895580.1pmspect.line.eqWidthAb189558[]? Abundance for the star HD 189558 (1)phys.abundEW193901[]? Equivalent width for the star HD 1939010.1pmspect.line.eqWidthAb193901[]? Abundance for the star HD 193901 (1)phys.abundEW194598[]? Equivalent width for the star HD 1945980.1pmspect.line.eqWidthAb194598[]? Abundance for the star HD 194598 (1)phys.abundEW196892[]? Equivalent width for the star HD 1968920.1pmspect.line.eqWidthAb196892[]? Abundance for the star HD 196892 (1)phys.abundEW199289[]? Equivalent width for the star HD 1992890.1pmspect.line.eqWidthAb199289[]? Abundance for the star HD 199289 (1)phys.abund
ivo://CDS.VizieR/J/A+A/306/1342019-06-21T18:30:00ZJ.A_Aivo_managed1Liller 1 (Ortolani+, 1996)J/A+A/306/134ivo://CDS.VizieR/J/A+A/306/134CDSOrtolani S., Bica E., Barbuy B.Simona Mei [CDS]1997-12-09T17:38:5705-Jul-1995CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.frGlobular_ClustersWe carried out VRI and Gunn z observations of the obscured globular cluster Liller 1. The cluster is so reddened (A_V_=~9.0) that it is at the detection limit in V. The RGB in I vs. (I-z) shows a strong curvature. Recalling that the nearly solar metallicity globular clusters NGC 6553 and NGC 6528 present similar blanketing effects only in the visible bandpasses, we conclude that Liller 1 is considerably more metal-rich than these clusters. The CMD comparison of Liller 1 with the inner bulge field around it (located =~5deg from the nucleus), suggests that the cluster is as metallic as the most metallic fraction of this inner bulge population. Similarly deep I and z observations at =~0.5deg away from Liller 1, at the nominal position of Grindlay 1 do not reveal any cluster. http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/306/134CatalogResearchIsServedByTAP VizieR generic servicepublichttp://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=J/A+A/306/134http://vizier.u-strasbg.fr/viz-bin/votable/-dtd/-A?-source=J/A+A/306/134GETtext/xml+votablehttp://tapvizier.u-strasbg.fr/TAPVizieR/tapOpticalInfrared
J/A+A/306/134/table2I, Gunn z photometry of Liller1recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordNumber+ Sequence numbermeta.id;meta.mainXposX pixel coordinatepixpos.cartesian.x;instr.detYposY pixel coordinatepixpos.cartesian.y;instr.detImagI magnitudesmagphot.mag;em.opt.IGmagGunn z instrumental magnitudesmagphot.mag;em.opt.IRDistRadial distance to cluster centerpixpos.cartesian;instr.det